The Macquarie/AAO/Strasbourg Hα Planetary Nebula Catalogue: MASH
Identifieur interne : 002366 ( Istex/Corpus ); précédent : 002365; suivant : 002367The Macquarie/AAO/Strasbourg Hα Planetary Nebula Catalogue: MASH
Auteurs : Quentin A. Parker ; A. Acker ; D. J. Frew ; M. Hartley ; A. E. J. Peyaud ; F. Ochsenbein ; S. Phillipps ; D. Russeil ; S. F. Beaulieu ; M. Cohen ; J. Köppen ; B. Miszalski ; D. H. Morgan ; R. A. H. Morris ; M. J. Pierce ; A. E. VaughanSource :
- Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 2006-11-21.
English descriptors
- KwdEn :
- Accurate positions, Acker, Acker stenholm, Angular extent, Arcmin2, Arcmin2 extracts, Arcsec, Arcsecond resolution, Astron, Astronomical tools, Basic plots, Bipolar, Bottom panel, Brief description, Bulge, Bulge region, Catalogue, Central star, Central stars, Central wavelength, Chemical enrichment, Clickable link, Colour, Colour image, Column entries, Compact emitters, Conf, Considerable overlap, Corradi, Corradi schwarz, Cspn, Cspn candidates, Current mash, Data base, Difference imaging, Different telescopes, Digital data, Discrete sources, Edinburgh university, Eld, Entire sample, Extensive programme, Flair flair, Frew, Frew parker, Further work, Galactic, Galactic bulge, Galactic latitude, Galactic latitude histograms, Galactic longitude, Galactic plane, Galaxy, Geometric centre, Hambly, Homogeneous sample, Imaging, Internal structure bottom column, Iras colours, Journal compilation, Kerber, Kohoutek, Large fraction, Line ratios, Louis pasteur, Lower surface brightness, Lter, Lter bandpass, Luminosity function, Macquarie, Macquarie univ, Macquarie university, Madsen frew, Main mash catalogue, Major axis dimension, Mash, Mash bulge, Mash catalogue, Mash catalogues, Mash data base, Mash discoveries, Mash histograms, Mash sample, Mgren spheres, Middle column, Minor axis, Miscellaneous emission nebulae, Mnras, Morphology, Mssso, Mssso observations, National science foundation, Nebula, Nebular, Nebular contamination, Observational data, Obvious cspn, Ongoing programme, Online, Optical spectroscopy, Other criteria, Parameter space, Parker morgan, Parker phillipps, Parker russeil, Peyaud, Photometric information, Pixel data, Planetary nebula catalogue, Planetary nebulae, Plots show, Previous catalogues, Previous samples, Previous surveys, Proc, Programme, Quotient, Retha pretorius, Rich bulge, Saao, Same telescope, Schmidt telescope, Schwarz, Spec, Spectral signatures, Spectroscopic, Spectroscopy, Stellar evolution, Stenholm, Such candidates, Such cases, Summary details, Summary page, Supercosmos, Supercosmos data, Surface brightness, Survey atlas, Survey data, Survey images, Symbiotic stars, Telescope, Tweedy, Tweedy kwitter, Ukst, Vast majority, Visual scanning, Visual scans, Visual search, Wavelength coverage, Weinberger, Zijlstra pottasch.
- Teeft :
- Accurate positions, Acker, Acker stenholm, Angular extent, Arcmin2, Arcmin2 extracts, Arcsec, Arcsecond resolution, Astron, Astronomical tools, Basic plots, Bipolar, Bottom panel, Brief description, Bulge, Bulge region, Catalogue, Central star, Central stars, Central wavelength, Chemical enrichment, Clickable link, Colour, Colour image, Column entries, Compact emitters, Conf, Considerable overlap, Corradi, Corradi schwarz, Cspn, Cspn candidates, Current mash, Data base, Difference imaging, Different telescopes, Digital data, Discrete sources, Edinburgh university, Eld, Entire sample, Extensive programme, Flair flair, Frew, Frew parker, Further work, Galactic, Galactic bulge, Galactic latitude, Galactic latitude histograms, Galactic longitude, Galactic plane, Galaxy, Geometric centre, Hambly, Homogeneous sample, Imaging, Internal structure bottom column, Iras colours, Journal compilation, Kerber, Kohoutek, Large fraction, Line ratios, Louis pasteur, Lower surface brightness, Lter, Lter bandpass, Luminosity function, Macquarie, Macquarie univ, Macquarie university, Madsen frew, Main mash catalogue, Major axis dimension, Mash, Mash bulge, Mash catalogue, Mash catalogues, Mash data base, Mash discoveries, Mash histograms, Mash sample, Mgren spheres, Middle column, Minor axis, Miscellaneous emission nebulae, Mnras, Morphology, Mssso, Mssso observations, National science foundation, Nebula, Nebular, Nebular contamination, Observational data, Obvious cspn, Ongoing programme, Online, Optical spectroscopy, Other criteria, Parameter space, Parker morgan, Parker phillipps, Parker russeil, Peyaud, Photometric information, Pixel data, Planetary nebula catalogue, Planetary nebulae, Plots show, Previous catalogues, Previous samples, Previous surveys, Proc, Programme, Quotient, Retha pretorius, Rich bulge, Saao, Same telescope, Schmidt telescope, Schwarz, Spec, Spectral signatures, Spectroscopic, Spectroscopy, Stellar evolution, Stenholm, Such candidates, Such cases, Summary details, Summary page, Supercosmos, Supercosmos data, Surface brightness, Survey atlas, Survey data, Survey images, Symbiotic stars, Telescope, Tweedy, Tweedy kwitter, Ukst, Vast majority, Visual scanning, Visual scans, Visual search, Wavelength coverage, Weinberger, Zijlstra pottasch.
Abstract
We present the Macquarie/AAO/Strasbourg Hα Planetary Nebula Catalogue (MASH) of over 900 true, likely and possible new Galactic planetary nebulae (PNe) discovered from the AAO/UKST Hα survey of the southern Galactic plane. The combination of depth, resolution, uniformity and areal coverage of the Hα survey has opened up a hitherto unexplored region of parameter space permitting the detection of this significant new PN sample. Away from the Galactic bulge the new PNe are typically more evolved, of larger angular extent, of lower surface brightness and more obscured (i.e. extinguished) than those in most previous surveys. We have also doubled the number of PNe in the Galactic bulge itself and although most are compact, we have also found more evolved examples. The MASH catalogue represents the culmination of a seven‐year programme of identification and confirmatory spectroscopy. A key strength is that the entire sample has been derived from the same, uniform observational data. The 60 per cent increase in known Galactic PNe represents the largest ever incremental sample of such discoveries and will have a significant impact on many aspects of PN research. This is especially important for studies at the faint end of the PN luminosity function which was previously poorly represented.
Url:
DOI: 10.1111/j.1365-2966.2006.10950.x
Links to Exploration step
ISTEX:BF6D77B88884A9AF8CA9C5B5F0B6FAD2D9A8515ALe document en format XML
<record><TEI wicri:istexFullTextTei="biblStruct"><teiHeader><fileDesc><titleStmt><title xml:lang="en">The Macquarie/AAO/Strasbourg Hα Planetary Nebula Catalogue: MASH</title><author><name sortKey="Parker, Quentin A" sort="Parker, Quentin A" uniqKey="Parker Q" first="Quentin A." last="Parker">Quentin A. Parker</name><affiliation><mods:affiliation>Department of Physics, Macquarie University, Sydney, NSW 2109, Australia</mods:affiliation></affiliation><affiliation><mods:affiliation>Anglo‐Australian Observatory, Epping, NSW 1710, Australia</mods:affiliation></affiliation><affiliation><mods:affiliation>E-mail: qap@ics.mq.edu.au</mods:affiliation></affiliation></author><author><name sortKey="Acker, A" sort="Acker, A" uniqKey="Acker A" first="A." last="Acker">A. Acker</name><affiliation><mods:affiliation>Observatoire Astronomique, Université Louis Pasteur, 67000 Strasbourg, France</mods:affiliation></affiliation></author><author><name sortKey="Frew, D J" sort="Frew, D J" uniqKey="Frew D" first="D. J." last="Frew">D. J. Frew</name><affiliation><mods:affiliation>Department of Physics, Macquarie University, Sydney, NSW 2109, Australia</mods:affiliation></affiliation></author><author><name sortKey="Hartley, M" sort="Hartley, M" uniqKey="Hartley M" first="M." last="Hartley">M. Hartley</name><affiliation><mods:affiliation>UK Schmidt Telescope, Anglo‐Australian Observatory, Siding Spring, 2357 NSW, Australia</mods:affiliation></affiliation></author><author><name sortKey="Peyaud, A E J" sort="Peyaud, A E J" uniqKey="Peyaud A" first="A. E. J." last="Peyaud">A. E. J. Peyaud</name><affiliation><mods:affiliation>Department of Physics, Macquarie University, Sydney, NSW 2109, Australia</mods:affiliation></affiliation><affiliation><mods:affiliation>Observatoire Astronomique, Université Louis Pasteur, 67000 Strasbourg, France</mods:affiliation></affiliation></author><author><name sortKey="Ochsenbein, F" sort="Ochsenbein, F" uniqKey="Ochsenbein F" first="F." last="Ochsenbein">F. Ochsenbein</name><affiliation><mods:affiliation>Observatoire Astronomique, Université Louis Pasteur, 67000 Strasbourg, France</mods:affiliation></affiliation></author><author><name sortKey="Phillipps, S" sort="Phillipps, S" uniqKey="Phillipps S" first="S." last="Phillipps">S. Phillipps</name><affiliation><mods:affiliation>Astrophysics Group, University of Bristol, Tyndall Avenue, Bristol BS8 1TL</mods:affiliation></affiliation></author><author><name sortKey="Russeil, D" sort="Russeil, D" uniqKey="Russeil D" first="D." last="Russeil">D. Russeil</name><affiliation><mods:affiliation>Laboratoire d'Astrophysique de Marseille, 2 Place Le Verrier, 13248 Marseille Cedex 04, France</mods:affiliation></affiliation></author><author><name sortKey="Beaulieu, S F" sort="Beaulieu, S F" uniqKey="Beaulieu S" first="S. F." last="Beaulieu">S. F. Beaulieu</name><affiliation><mods:affiliation>Département de Physique, et Observatoire du mont Mégantic, Université Laval, Québec, QC, Canada G1K 7P4</mods:affiliation></affiliation></author><author><name sortKey="Cohen, M" sort="Cohen, M" uniqKey="Cohen M" first="M." last="Cohen">M. Cohen</name><affiliation><mods:affiliation>Radio Astronomy Laboratory, University of California, Berkeley, CA 94720, USA</mods:affiliation></affiliation></author><author><name sortKey="Koppen, J" sort="Koppen, J" uniqKey="Koppen J" first="J." last="Köppen">J. Köppen</name><affiliation><mods:affiliation>Observatoire Astronomique, Université Louis Pasteur, 67000 Strasbourg, France</mods:affiliation></affiliation></author><author><name sortKey="Miszalski, B" sort="Miszalski, B" uniqKey="Miszalski B" first="B." last="Miszalski">B. Miszalski</name><affiliation><mods:affiliation>Department of Physics, Macquarie University, Sydney, NSW 2109, Australia</mods:affiliation></affiliation></author><author><name sortKey="Morgan, D H" sort="Morgan, D H" uniqKey="Morgan D" first="D. H." last="Morgan">D. H. Morgan</name><affiliation><mods:affiliation>Institute for Astronomy, School of Physics, University of Edinburgh, Edinburgh EH8 3HJ</mods:affiliation></affiliation></author><author><name sortKey="Morris, R A H" sort="Morris, R A H" uniqKey="Morris R" first="R. A. H." last="Morris">R. A. H. Morris</name><affiliation><mods:affiliation>Astrophysics Group, University of Bristol, Tyndall Avenue, Bristol BS8 1TL</mods:affiliation></affiliation></author><author><name sortKey="Pierce, M J" sort="Pierce, M J" uniqKey="Pierce M" first="M. J." last="Pierce">M. J. Pierce</name><affiliation><mods:affiliation>Department of Physics, Macquarie University, Sydney, NSW 2109, Australia</mods:affiliation></affiliation><affiliation><mods:affiliation>Astrophysics Group, University of Bristol, Tyndall Avenue, Bristol BS8 1TL</mods:affiliation></affiliation></author><author><name sortKey="Vaughan, A E" sort="Vaughan, A E" uniqKey="Vaughan A" first="A. E." last="Vaughan">A. E. Vaughan</name><affiliation><mods:affiliation>Department of Physics, Macquarie University, Sydney, NSW 2109, Australia</mods:affiliation></affiliation></author></titleStmt><publicationStmt><idno type="wicri:source">ISTEX</idno><idno type="RBID">ISTEX:BF6D77B88884A9AF8CA9C5B5F0B6FAD2D9A8515A</idno><date when="2006" year="2006">2006</date><idno type="doi">10.1111/j.1365-2966.2006.10950.x</idno><idno type="url">https://api.istex.fr/document/BF6D77B88884A9AF8CA9C5B5F0B6FAD2D9A8515A/fulltext/pdf</idno><idno type="wicri:Area/Istex/Corpus">002366</idno><idno type="wicri:explorRef" wicri:stream="Istex" wicri:step="Corpus" wicri:corpus="ISTEX">002366</idno></publicationStmt><sourceDesc><biblStruct><analytic><title level="a" type="main">The Macquarie/AAO/Strasbourg Hα Planetary Nebula Catalogue: MASH</title><author><name sortKey="Parker, Quentin A" sort="Parker, Quentin A" uniqKey="Parker Q" first="Quentin A." last="Parker">Quentin A. Parker</name><affiliation><mods:affiliation>Department of Physics, Macquarie University, Sydney, NSW 2109, Australia</mods:affiliation></affiliation><affiliation><mods:affiliation>Anglo‐Australian Observatory, Epping, NSW 1710, Australia</mods:affiliation></affiliation><affiliation><mods:affiliation>E-mail: qap@ics.mq.edu.au</mods:affiliation></affiliation></author><author><name sortKey="Acker, A" sort="Acker, A" uniqKey="Acker A" first="A." last="Acker">A. Acker</name><affiliation><mods:affiliation>Observatoire Astronomique, Université Louis Pasteur, 67000 Strasbourg, France</mods:affiliation></affiliation></author><author><name sortKey="Frew, D J" sort="Frew, D J" uniqKey="Frew D" first="D. J." last="Frew">D. J. Frew</name><affiliation><mods:affiliation>Department of Physics, Macquarie University, Sydney, NSW 2109, Australia</mods:affiliation></affiliation></author><author><name sortKey="Hartley, M" sort="Hartley, M" uniqKey="Hartley M" first="M." last="Hartley">M. Hartley</name><affiliation><mods:affiliation>UK Schmidt Telescope, Anglo‐Australian Observatory, Siding Spring, 2357 NSW, Australia</mods:affiliation></affiliation></author><author><name sortKey="Peyaud, A E J" sort="Peyaud, A E J" uniqKey="Peyaud A" first="A. E. J." last="Peyaud">A. E. J. Peyaud</name><affiliation><mods:affiliation>Department of Physics, Macquarie University, Sydney, NSW 2109, Australia</mods:affiliation></affiliation><affiliation><mods:affiliation>Observatoire Astronomique, Université Louis Pasteur, 67000 Strasbourg, France</mods:affiliation></affiliation></author><author><name sortKey="Ochsenbein, F" sort="Ochsenbein, F" uniqKey="Ochsenbein F" first="F." last="Ochsenbein">F. Ochsenbein</name><affiliation><mods:affiliation>Observatoire Astronomique, Université Louis Pasteur, 67000 Strasbourg, France</mods:affiliation></affiliation></author><author><name sortKey="Phillipps, S" sort="Phillipps, S" uniqKey="Phillipps S" first="S." last="Phillipps">S. Phillipps</name><affiliation><mods:affiliation>Astrophysics Group, University of Bristol, Tyndall Avenue, Bristol BS8 1TL</mods:affiliation></affiliation></author><author><name sortKey="Russeil, D" sort="Russeil, D" uniqKey="Russeil D" first="D." last="Russeil">D. Russeil</name><affiliation><mods:affiliation>Laboratoire d'Astrophysique de Marseille, 2 Place Le Verrier, 13248 Marseille Cedex 04, France</mods:affiliation></affiliation></author><author><name sortKey="Beaulieu, S F" sort="Beaulieu, S F" uniqKey="Beaulieu S" first="S. F." last="Beaulieu">S. F. Beaulieu</name><affiliation><mods:affiliation>Département de Physique, et Observatoire du mont Mégantic, Université Laval, Québec, QC, Canada G1K 7P4</mods:affiliation></affiliation></author><author><name sortKey="Cohen, M" sort="Cohen, M" uniqKey="Cohen M" first="M." last="Cohen">M. Cohen</name><affiliation><mods:affiliation>Radio Astronomy Laboratory, University of California, Berkeley, CA 94720, USA</mods:affiliation></affiliation></author><author><name sortKey="Koppen, J" sort="Koppen, J" uniqKey="Koppen J" first="J." last="Köppen">J. Köppen</name><affiliation><mods:affiliation>Observatoire Astronomique, Université Louis Pasteur, 67000 Strasbourg, France</mods:affiliation></affiliation></author><author><name sortKey="Miszalski, B" sort="Miszalski, B" uniqKey="Miszalski B" first="B." last="Miszalski">B. Miszalski</name><affiliation><mods:affiliation>Department of Physics, Macquarie University, Sydney, NSW 2109, Australia</mods:affiliation></affiliation></author><author><name sortKey="Morgan, D H" sort="Morgan, D H" uniqKey="Morgan D" first="D. H." last="Morgan">D. H. Morgan</name><affiliation><mods:affiliation>Institute for Astronomy, School of Physics, University of Edinburgh, Edinburgh EH8 3HJ</mods:affiliation></affiliation></author><author><name sortKey="Morris, R A H" sort="Morris, R A H" uniqKey="Morris R" first="R. A. H." last="Morris">R. A. H. Morris</name><affiliation><mods:affiliation>Astrophysics Group, University of Bristol, Tyndall Avenue, Bristol BS8 1TL</mods:affiliation></affiliation></author><author><name sortKey="Pierce, M J" sort="Pierce, M J" uniqKey="Pierce M" first="M. J." last="Pierce">M. J. Pierce</name><affiliation><mods:affiliation>Department of Physics, Macquarie University, Sydney, NSW 2109, Australia</mods:affiliation></affiliation><affiliation><mods:affiliation>Astrophysics Group, University of Bristol, Tyndall Avenue, Bristol BS8 1TL</mods:affiliation></affiliation></author><author><name sortKey="Vaughan, A E" sort="Vaughan, A E" uniqKey="Vaughan A" first="A. E." last="Vaughan">A. E. Vaughan</name><affiliation><mods:affiliation>Department of Physics, Macquarie University, Sydney, NSW 2109, Australia</mods:affiliation></affiliation></author></analytic><monogr></monogr><series><title level="j" type="main">Monthly Notices of the Royal Astronomical Society</title><title level="j" type="alt">MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY</title><idno type="ISSN">0035-8711</idno><idno type="eISSN">1365-2966</idno><imprint><biblScope unit="vol">373</biblScope><biblScope unit="issue">1</biblScope><biblScope unit="page" from="79">79</biblScope><biblScope unit="page" to="94">94</biblScope><biblScope unit="page-count">16</biblScope><publisher>Blackwell Publishing Ltd</publisher><pubPlace>Oxford, UK</pubPlace><date type="published" when="2006-11-21">2006-11-21</date></imprint><idno type="ISSN">0035-8711</idno></series></biblStruct></sourceDesc><seriesStmt><idno type="ISSN">0035-8711</idno></seriesStmt></fileDesc><profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>Accurate positions</term><term>Acker</term><term>Acker stenholm</term><term>Angular extent</term><term>Arcmin2</term><term>Arcmin2 extracts</term><term>Arcsec</term><term>Arcsecond resolution</term><term>Astron</term><term>Astronomical tools</term><term>Basic plots</term><term>Bipolar</term><term>Bottom panel</term><term>Brief description</term><term>Bulge</term><term>Bulge region</term><term>Catalogue</term><term>Central star</term><term>Central stars</term><term>Central wavelength</term><term>Chemical enrichment</term><term>Clickable link</term><term>Colour</term><term>Colour image</term><term>Column entries</term><term>Compact emitters</term><term>Conf</term><term>Considerable overlap</term><term>Corradi</term><term>Corradi schwarz</term><term>Cspn</term><term>Cspn candidates</term><term>Current mash</term><term>Data base</term><term>Difference imaging</term><term>Different telescopes</term><term>Digital data</term><term>Discrete sources</term><term>Edinburgh university</term><term>Eld</term><term>Entire sample</term><term>Extensive programme</term><term>Flair flair</term><term>Frew</term><term>Frew parker</term><term>Further work</term><term>Galactic</term><term>Galactic bulge</term><term>Galactic latitude</term><term>Galactic latitude histograms</term><term>Galactic longitude</term><term>Galactic plane</term><term>Galaxy</term><term>Geometric centre</term><term>Hambly</term><term>Homogeneous sample</term><term>Imaging</term><term>Internal structure bottom column</term><term>Iras colours</term><term>Journal compilation</term><term>Kerber</term><term>Kohoutek</term><term>Large fraction</term><term>Line ratios</term><term>Louis pasteur</term><term>Lower surface brightness</term><term>Lter</term><term>Lter bandpass</term><term>Luminosity function</term><term>Macquarie</term><term>Macquarie univ</term><term>Macquarie university</term><term>Madsen frew</term><term>Main mash catalogue</term><term>Major axis dimension</term><term>Mash</term><term>Mash bulge</term><term>Mash catalogue</term><term>Mash catalogues</term><term>Mash data base</term><term>Mash discoveries</term><term>Mash histograms</term><term>Mash sample</term><term>Mgren spheres</term><term>Middle column</term><term>Minor axis</term><term>Miscellaneous emission nebulae</term><term>Mnras</term><term>Morphology</term><term>Mssso</term><term>Mssso observations</term><term>National science foundation</term><term>Nebula</term><term>Nebular</term><term>Nebular contamination</term><term>Observational data</term><term>Obvious cspn</term><term>Ongoing programme</term><term>Online</term><term>Optical spectroscopy</term><term>Other criteria</term><term>Parameter space</term><term>Parker morgan</term><term>Parker phillipps</term><term>Parker russeil</term><term>Peyaud</term><term>Photometric information</term><term>Pixel data</term><term>Planetary nebula catalogue</term><term>Planetary nebulae</term><term>Plots show</term><term>Previous catalogues</term><term>Previous samples</term><term>Previous surveys</term><term>Proc</term><term>Programme</term><term>Quotient</term><term>Retha pretorius</term><term>Rich bulge</term><term>Saao</term><term>Same telescope</term><term>Schmidt telescope</term><term>Schwarz</term><term>Spec</term><term>Spectral signatures</term><term>Spectroscopic</term><term>Spectroscopy</term><term>Stellar evolution</term><term>Stenholm</term><term>Such candidates</term><term>Such cases</term><term>Summary details</term><term>Summary page</term><term>Supercosmos</term><term>Supercosmos data</term><term>Surface brightness</term><term>Survey atlas</term><term>Survey data</term><term>Survey images</term><term>Symbiotic stars</term><term>Telescope</term><term>Tweedy</term><term>Tweedy kwitter</term><term>Ukst</term><term>Vast majority</term><term>Visual scanning</term><term>Visual scans</term><term>Visual search</term><term>Wavelength coverage</term><term>Weinberger</term><term>Zijlstra pottasch</term></keywords><keywords scheme="Teeft" xml:lang="en"><term>Accurate positions</term><term>Acker</term><term>Acker stenholm</term><term>Angular extent</term><term>Arcmin2</term><term>Arcmin2 extracts</term><term>Arcsec</term><term>Arcsecond resolution</term><term>Astron</term><term>Astronomical tools</term><term>Basic plots</term><term>Bipolar</term><term>Bottom panel</term><term>Brief description</term><term>Bulge</term><term>Bulge region</term><term>Catalogue</term><term>Central star</term><term>Central stars</term><term>Central wavelength</term><term>Chemical enrichment</term><term>Clickable link</term><term>Colour</term><term>Colour image</term><term>Column entries</term><term>Compact emitters</term><term>Conf</term><term>Considerable overlap</term><term>Corradi</term><term>Corradi schwarz</term><term>Cspn</term><term>Cspn candidates</term><term>Current mash</term><term>Data base</term><term>Difference imaging</term><term>Different telescopes</term><term>Digital data</term><term>Discrete sources</term><term>Edinburgh university</term><term>Eld</term><term>Entire sample</term><term>Extensive programme</term><term>Flair flair</term><term>Frew</term><term>Frew parker</term><term>Further work</term><term>Galactic</term><term>Galactic bulge</term><term>Galactic latitude</term><term>Galactic latitude histograms</term><term>Galactic longitude</term><term>Galactic plane</term><term>Galaxy</term><term>Geometric centre</term><term>Hambly</term><term>Homogeneous sample</term><term>Imaging</term><term>Internal structure bottom column</term><term>Iras colours</term><term>Journal compilation</term><term>Kerber</term><term>Kohoutek</term><term>Large fraction</term><term>Line ratios</term><term>Louis pasteur</term><term>Lower surface brightness</term><term>Lter</term><term>Lter bandpass</term><term>Luminosity function</term><term>Macquarie</term><term>Macquarie univ</term><term>Macquarie university</term><term>Madsen frew</term><term>Main mash catalogue</term><term>Major axis dimension</term><term>Mash</term><term>Mash bulge</term><term>Mash catalogue</term><term>Mash catalogues</term><term>Mash data base</term><term>Mash discoveries</term><term>Mash histograms</term><term>Mash sample</term><term>Mgren spheres</term><term>Middle column</term><term>Minor axis</term><term>Miscellaneous emission nebulae</term><term>Mnras</term><term>Morphology</term><term>Mssso</term><term>Mssso observations</term><term>National science foundation</term><term>Nebula</term><term>Nebular</term><term>Nebular contamination</term><term>Observational data</term><term>Obvious cspn</term><term>Ongoing programme</term><term>Online</term><term>Optical spectroscopy</term><term>Other criteria</term><term>Parameter space</term><term>Parker morgan</term><term>Parker phillipps</term><term>Parker russeil</term><term>Peyaud</term><term>Photometric information</term><term>Pixel data</term><term>Planetary nebula catalogue</term><term>Planetary nebulae</term><term>Plots show</term><term>Previous catalogues</term><term>Previous samples</term><term>Previous surveys</term><term>Proc</term><term>Programme</term><term>Quotient</term><term>Retha pretorius</term><term>Rich bulge</term><term>Saao</term><term>Same telescope</term><term>Schmidt telescope</term><term>Schwarz</term><term>Spec</term><term>Spectral signatures</term><term>Spectroscopic</term><term>Spectroscopy</term><term>Stellar evolution</term><term>Stenholm</term><term>Such candidates</term><term>Such cases</term><term>Summary details</term><term>Summary page</term><term>Supercosmos</term><term>Supercosmos data</term><term>Surface brightness</term><term>Survey atlas</term><term>Survey data</term><term>Survey images</term><term>Symbiotic stars</term><term>Telescope</term><term>Tweedy</term><term>Tweedy kwitter</term><term>Ukst</term><term>Vast majority</term><term>Visual scanning</term><term>Visual scans</term><term>Visual search</term><term>Wavelength coverage</term><term>Weinberger</term><term>Zijlstra pottasch</term></keywords></textClass></profileDesc></teiHeader><front><div type="abstract" xml:lang="en">We present the Macquarie/AAO/Strasbourg Hα Planetary Nebula Catalogue (MASH) of over 900 true, likely and possible new Galactic planetary nebulae (PNe) discovered from the AAO/UKST Hα survey of the southern Galactic plane. The combination of depth, resolution, uniformity and areal coverage of the Hα survey has opened up a hitherto unexplored region of parameter space permitting the detection of this significant new PN sample. Away from the Galactic bulge the new PNe are typically more evolved, of larger angular extent, of lower surface brightness and more obscured (i.e. extinguished) than those in most previous surveys. We have also doubled the number of PNe in the Galactic bulge itself and although most are compact, we have also found more evolved examples. The MASH catalogue represents the culmination of a seven‐year programme of identification and confirmatory spectroscopy. A key strength is that the entire sample has been derived from the same, uniform observational data. The 60 per cent increase in known Galactic PNe represents the largest ever incremental sample of such discoveries and will have a significant impact on many aspects of PN research. This is especially important for studies at the faint end of the PN luminosity function which was previously poorly represented.</div></front></TEI><istex><corpusName>wiley</corpusName><keywords><teeft><json:string>mash</json:string><json:string>nebula</json:string><json:string>acker</json:string><json:string>mnras</json:string><json:string>cspn</json:string><json:string>arcsec</json:string><json:string>galactic</json:string><json:string>eld</json:string><json:string>supercosmos</json:string><json:string>corradi</json:string><json:string>mssso</json:string><json:string>ukst</json:string><json:string>journal compilation</json:string><json:string>frew</json:string><json:string>saao</json:string><json:string>peyaud</json:string><json:string>spectroscopic</json:string><json:string>mash catalogue</json:string><json:string>stenholm</json:string><json:string>programme</json:string><json:string>bipolar</json:string><json:string>kohoutek</json:string><json:string>galactic bulge</json:string><json:string>planetary nebula catalogue</json:string><json:string>schwarz</json:string><json:string>astron</json:string><json:string>kerber</json:string><json:string>online</json:string><json:string>difference imaging</json:string><json:string>planetary nebulae</json:string><json:string>quotient</json:string><json:string>conf</json:string><json:string>lter</json:string><json:string>macquarie</json:string><json:string>proc</json:string><json:string>weinberger</json:string><json:string>arcmin2</json:string><json:string>colour</json:string><json:string>central star</json:string><json:string>hambly</json:string><json:string>surface brightness</json:string><json:string>macquarie university</json:string><json:string>galactic plane</json:string><json:string>line ratios</json:string><json:string>imaging</json:string><json:string>catalogue</json:string><json:string>spec</json:string><json:string>bulge</json:string><json:string>survey data</json:string><json:string>central stars</json:string><json:string>galactic latitude</json:string><json:string>mash sample</json:string><json:string>cspn candidates</json:string><json:string>summary page</json:string><json:string>supercosmos data</json:string><json:string>frew parker</json:string><json:string>nebular</json:string><json:string>morphology</json:string><json:string>tweedy</json:string><json:string>previous catalogues</json:string><json:string>symbiotic stars</json:string><json:string>acker stenholm</json:string><json:string>visual scans</json:string><json:string>pixel data</json:string><json:string>digital data</json:string><json:string>corradi schwarz</json:string><json:string>data base</json:string><json:string>louis pasteur</json:string><json:string>stellar evolution</json:string><json:string>main mash catalogue</json:string><json:string>different telescopes</json:string><json:string>galactic longitude</json:string><json:string>wavelength coverage</json:string><json:string>bottom panel</json:string><json:string>plots show</json:string><json:string>mash catalogues</json:string><json:string>luminosity function</json:string><json:string>mash data base</json:string><json:string>spectroscopy</json:string><json:string>telescope</json:string><json:string>extensive programme</json:string><json:string>optical spectroscopy</json:string><json:string>other criteria</json:string><json:string>tweedy kwitter</json:string><json:string>same telescope</json:string><json:string>astronomical tools</json:string><json:string>rich bulge</json:string><json:string>iras colours</json:string><json:string>summary details</json:string><json:string>visual scanning</json:string><json:string>such candidates</json:string><json:string>flair flair</json:string><json:string>homogeneous sample</json:string><json:string>arcmin2 extracts</json:string><json:string>mssso observations</json:string><json:string>parker morgan</json:string><json:string>such cases</json:string><json:string>schmidt telescope</json:string><json:string>spectral signatures</json:string><json:string>mgren spheres</json:string><json:string>current mash</json:string><json:string>considerable overlap</json:string><json:string>further work</json:string><json:string>madsen frew</json:string><json:string>macquarie univ</json:string><json:string>discrete sources</json:string><json:string>entire sample</json:string><json:string>lower surface brightness</json:string><json:string>lter bandpass</json:string><json:string>miscellaneous emission nebulae</json:string><json:string>photometric information</json:string><json:string>central wavelength</json:string><json:string>parker phillipps</json:string><json:string>brief description</json:string><json:string>previous surveys</json:string><json:string>clickable link</json:string><json:string>column entries</json:string><json:string>colour image</json:string><json:string>accurate positions</json:string><json:string>obvious cspn</json:string><json:string>vast majority</json:string><json:string>mash discoveries</json:string><json:string>retha pretorius</json:string><json:string>angular extent</json:string><json:string>large fraction</json:string><json:string>geometric centre</json:string><json:string>zijlstra pottasch</json:string><json:string>minor axis</json:string><json:string>previous samples</json:string><json:string>arcsecond resolution</json:string><json:string>major axis dimension</json:string><json:string>mash bulge</json:string><json:string>basic plots</json:string><json:string>parameter space</json:string><json:string>galactic latitude histograms</json:string><json:string>observational data</json:string><json:string>bulge region</json:string><json:string>mash histograms</json:string><json:string>internal structure bottom column</json:string><json:string>nebular contamination</json:string><json:string>ongoing programme</json:string><json:string>survey atlas</json:string><json:string>chemical enrichment</json:string><json:string>parker russeil</json:string><json:string>edinburgh university</json:string><json:string>national science foundation</json:string><json:string>survey images</json:string><json:string>visual search</json:string><json:string>middle column</json:string><json:string>compact emitters</json:string><json:string>galaxy</json:string></teeft></keywords><author><json:item><name>Quentin A. Parker</name><affiliations><json:string>Department of Physics, Macquarie University, Sydney, NSW 2109, Australia</json:string><json:string>Anglo‐Australian Observatory, Epping, NSW 1710, Australia</json:string><json:string>E-mail: qap@ics.mq.edu.au</json:string></affiliations></json:item><json:item><name>A. Acker</name><affiliations><json:string>Observatoire Astronomique, Université Louis Pasteur, 67000 Strasbourg, France</json:string></affiliations></json:item><json:item><name>D. J. Frew</name><affiliations><json:string>Department of Physics, Macquarie University, Sydney, NSW 2109, Australia</json:string></affiliations></json:item><json:item><name>M. Hartley</name><affiliations><json:string>UK Schmidt Telescope, Anglo‐Australian Observatory, Siding Spring, 2357 NSW, Australia</json:string></affiliations></json:item><json:item><name>A. E. J. Peyaud</name><affiliations><json:string>Department of Physics, Macquarie University, Sydney, NSW 2109, Australia</json:string><json:string>Observatoire Astronomique, Université Louis Pasteur, 67000 Strasbourg, France</json:string></affiliations></json:item><json:item><name>F. Ochsenbein</name><affiliations><json:string>Observatoire Astronomique, Université Louis Pasteur, 67000 Strasbourg, France</json:string></affiliations></json:item><json:item><name>S. Phillipps</name><affiliations><json:string>Astrophysics Group, University of Bristol, Tyndall Avenue, Bristol BS8 1TL</json:string></affiliations></json:item><json:item><name>D. Russeil</name><affiliations><json:string>Laboratoire d'Astrophysique de Marseille, 2 Place Le Verrier, 13248 Marseille Cedex 04, France</json:string></affiliations></json:item><json:item><name>S. F. Beaulieu</name><affiliations><json:string>Département de Physique, et Observatoire du mont Mégantic, Université Laval, Québec, QC, Canada G1K 7P4</json:string></affiliations></json:item><json:item><name>M. Cohen</name><affiliations><json:string>Radio Astronomy Laboratory, University of California, Berkeley, CA 94720, USA</json:string></affiliations></json:item><json:item><name>J. Köppen</name><affiliations><json:string>Observatoire Astronomique, Université Louis Pasteur, 67000 Strasbourg, France</json:string></affiliations></json:item><json:item><name>B. Miszalski</name><affiliations><json:string>Department of Physics, Macquarie University, Sydney, NSW 2109, Australia</json:string></affiliations></json:item><json:item><name>D. H. Morgan</name><affiliations><json:string>Institute for Astronomy, School of Physics, University of Edinburgh, Edinburgh EH8 3HJ</json:string></affiliations></json:item><json:item><name>R. A. H. Morris</name><affiliations><json:string>Astrophysics Group, University of Bristol, Tyndall Avenue, Bristol BS8 1TL</json:string></affiliations></json:item><json:item><name>M. J. Pierce</name><affiliations><json:string>Department of Physics, Macquarie University, Sydney, NSW 2109, Australia</json:string><json:string>Astrophysics Group, University of Bristol, Tyndall Avenue, Bristol BS8 1TL</json:string></affiliations></json:item><json:item><name>A. E. Vaughan</name><affiliations><json:string>Department of Physics, Macquarie University, Sydney, NSW 2109, Australia</json:string></affiliations></json:item></author><subject><json:item><lang><json:string>eng</json:string></lang><value>astronomical data bases: miscellaneous</value></json:item><json:item><lang><json:string>eng</json:string></lang><value>catalogues</value></json:item><json:item><lang><json:string>eng</json:string></lang><value>surveys</value></json:item><json:item><lang><json:string>eng</json:string></lang><value>planetary nebulae: general</value></json:item></subject><articleId><json:string>MNR10950</json:string></articleId><arkIstex>ark:/67375/WNG-50LL8RG4-5</arkIstex><language><json:string>eng</json:string></language><originalGenre><json:string>article</json:string></originalGenre><abstract>We present the Macquarie/AAO/Strasbourg Hα Planetary Nebula Catalogue (MASH) of over 900 true, likely and possible new Galactic planetary nebulae (PNe) discovered from the AAO/UKST Hα survey of the southern Galactic plane. The combination of depth, resolution, uniformity and areal coverage of the Hα survey has opened up a hitherto unexplored region of parameter space permitting the detection of this significant new PN sample. Away from the Galactic bulge the new PNe are typically more evolved, of larger angular extent, of lower surface brightness and more obscured (i.e. extinguished) than those in most previous surveys. We have also doubled the number of PNe in the Galactic bulge itself and although most are compact, we have also found more evolved examples. The MASH catalogue represents the culmination of a seven‐year programme of identification and confirmatory spectroscopy. A key strength is that the entire sample has been derived from the same, uniform observational data. The 60 per cent increase in known Galactic PNe represents the largest ever incremental sample of such discoveries and will have a significant impact on many aspects of PN research. This is especially important for studies at the faint end of the PN luminosity function which was previously poorly represented.</abstract><qualityIndicators><score>9.424</score><pdfWordCount>12298</pdfWordCount><pdfCharCount>69774</pdfCharCount><pdfVersion>1.3</pdfVersion><pdfPageCount>16</pdfPageCount><pdfPageSize>612 x 792 pts (letter)</pdfPageSize><refBibsNative>true</refBibsNative><abstractWordCount>202</abstractWordCount><abstractCharCount>1300</abstractCharCount><keywordCount>4</keywordCount></qualityIndicators><title>The Macquarie/AAO/Strasbourg Hα Planetary Nebula Catalogue: MASH</title><genre><json:string>article</json:string></genre><host><title>Monthly Notices of the Royal Astronomical Society</title><language><json:string>unknown</json:string></language><doi><json:string>10.1111/(ISSN)1365-2966</json:string></doi><issn><json:string>0035-8711</json:string></issn><eissn><json:string>1365-2966</json:string></eissn><publisherId><json:string>MNR</json:string></publisherId><volume>373</volume><issue>1</issue><pages><first>79</first><last>94</last><total>16</total></pages><genre><json:string>journal</json:string></genre></host><namedEntities><unitex><date><json:string>2001</json:string><json:string>1385</json:string><json:string>2006</json:string><json:string>1998</json:string><json:string>2002</json:string><json:string>1510</json:string><json:string>1100</json:string><json:string>2003</json:string><json:string>1500</json:string><json:string>2004</json:string></date><geogName></geogName><orgName><json:string>National Science Foundation</json:string><json:string>Australia Observatory, Epping, NSW</json:string><json:string>Anglo-Australian Observatory UK Schmidt Telescope</json:string><json:string>Radio Astronomy Laboratory, University of California, Berkeley, CA</json:string><json:string>University of Massachusetts</json:string><json:string>Infrared Processing and Analysis Center</json:string><json:string>California Institute of Technology</json:string><json:string>Institute for Astronomy, School of Physics, University of Edinburgh, Edinburgh EH</json:string><json:string>Macquarie University</json:string><json:string>Edinburgh University</json:string><json:string>Bristol University</json:string><json:string>University of Bristol</json:string><json:string>US National Science Foundation</json:string></orgName><orgName_funder></orgName_funder><orgName_provider></orgName_provider><persName><json:string>S. F. Beaulieu</json:string><json:string>A. Acker</json:string><json:string>Sky Survey</json:string><json:string>BI Cru</json:string><json:string>I. Lundstr</json:string><json:string>Ian Bond</json:string><json:string>Unit</json:string><json:string>Jean-Marie Hameury</json:string><json:string>Research</json:string><json:string>Strasbourg Observatory</json:string><json:string>A. E. Vaughan</json:string><json:string>Cheryl Simms</json:string><json:string>R. A. H. Morris</json:string><json:string>Sybil Kadel</json:string><json:string>Quentin A. Parker</json:string><json:string>Edward Thomson</json:string><json:string>Van de Steene</json:string><json:string>Amanda Norton</json:string><json:string>La Palma</json:string><json:string>Massumeh Guyanapeh</json:string><json:string>Ella Hopewell</json:string><json:string>Brian Boyle</json:string><json:string>Mark Birkinshaw</json:string><json:string>Russell Cannon</json:string><json:string>Macquarie University</json:string><json:string>Louis Pasteur</json:string><json:string>D. Russeil</json:string><json:string>Matt Jones</json:string><json:string>D. H. Morgan</json:string><json:string>M. J. Pierce</json:string><json:string>F. Ochsenbein</json:string><json:string>A. E. J. Peyaud</json:string><json:string>Laura Morgan</json:string><json:string>Laura Douglas</json:string><json:string>Caroline Thomson</json:string><json:string>Milorad Stupar</json:string><json:string>Anne Rowntree</json:string><json:string>Elise Laird</json:string><json:string>David Riddle</json:string><json:string>S. Phillipps</json:string></persName><placeName><json:string>Bristol</json:string><json:string>Australia</json:string><json:string>Edinburgh</json:string><json:string>Strasbourg</json:string><json:string>Berkeley</json:string><json:string>WELS</json:string><json:string>France</json:string><json:string>Marseille</json:string></placeName><ref_url><json:string>http://www.aao.gov.au/local/www/brent/pndr/</json:string></ref_url><ref_bibl><json:string>Tylenda, Acker & Stenholm 1993</json:string><json:string>Parker & Malin 1999</json:string><json:string>Kerber, Lercher & Weinberger 1996</json:string><json:string>Q. A. Parker et al.</json:string><json:string>Morgan, Parker & Russeil 2001</json:string><json:string>Pierce 2005</json:string><json:string>Iben 1995</json:string><json:string>Parker et al. 2003</json:string><json:string>Frew & Parker 2005</json:string><json:string>Schwarz (1995)</json:string><json:string>Stupar et al. 2006</json:string><json:string>Kennicutt et al. 2000</json:string><json:string>Maciel & Costa 2003</json:string><json:string>Corradi & Schwarz 1993</json:string><json:string>Tweedy & Napiwotzki 1994</json:string><json:string>Napiwotzki 1995</json:string><json:string>Tweedy & Kwitter 1996</json:string><json:string>Morgan, Parker & Cohen 2003</json:string><json:string>Watson, Parker & Miziarski 1998</json:string><json:string>Hambly, Irwin & MacGillivray 2001b</json:string><json:string>Ochsenbein et al.</json:string><json:string>Frew 2006</json:string><json:string>Hambly et al. 2001b</json:string><json:string>Corradi et al. 1999</json:string><json:string>Hewett et al. 2003</json:string><json:string>Henize 1967</json:string><json:string>Hopewell et al.</json:string><json:string>Cohen & Parker 2003</json:string><json:string>Frew, Parker & Russeil 2006</json:string><json:string>Peyaud et al. 2003, 2004</json:string><json:string>Reid & Parker 2006a,b</json:string><json:string>Manchado (2004)</json:string><json:string>Parker, Frew & Stupar 2004</json:string><json:string>Mader et al. 1999</json:string><json:string>Peyaud 2005</json:string><json:string>Beard, MacGillivray & Thanisch 1990</json:string><json:string>Ochsenbein, Bauer & Marcout 2000</json:string><json:string>Corradi 1995</json:string><json:string>Hambly et al. 2001a</json:string><json:string>Jeffery et al. (1996)</json:string><json:string>Acker et al. (1992, 1996)</json:string><json:string>Parker & BlandHawthorn 1998</json:string><json:string>Zijlstra & Pottasch 1991</json:string><json:string>Xilouris et al. 1996</json:string><json:string>Acker, Marcout & Ochsenbein 1996</json:string><json:string>Tweedy & Kwitter 1994</json:string><json:string>Kaler 1981</json:string><json:string>Parker & Bland-Hawthorn 1998</json:string><json:string>Kerber et al.</json:string><json:string>Chu et al. (2004)</json:string><json:string>Melmer & Weinberger 1990</json:string><json:string>Price et al. 2001</json:string><json:string>Pierce et al. 2004</json:string><json:string>Kohoutek 2002</json:string><json:string>Fesen, Blair & Kirshner 1985</json:string><json:string>Corradi et al. 2005</json:string><json:string>Ciardullo et al. (1999)</json:string><json:string>Parker et al. 2005</json:string><json:string>Taylor et al. 1996</json:string><json:string>PhD, 2005</json:string><json:string>Corradi et al. 1997</json:string><json:string>UK Schmidt Telescope, Anglo-Australian Observatory, Siding Spring, 2357</json:string><json:string>Tweedy, Martos & Noriega-Crespo 1995</json:string><json:string>Larios & Phillips 2005</json:string><json:string>Kohoutek 2001</json:string><json:string>Schmeja & Kimeswenger 2001</json:string><json:string>Parker & Morgan 2003</json:string><json:string>Kerber et al. 1998</json:string><json:string>Parker & Phillipps 1998</json:string><json:string>Parker et al.</json:string><json:string>Parker et al. 2001, 2003</json:string><json:string>Acker et al. (1992)</json:string><json:string>Peyaud, Acker & Parker 2003, 2004</json:string><json:string>Boumis et al. (2003)</json:string><json:string>Gaustad et al. (2001)</json:string><json:string>Kraan-Korteweg et al. (1996)</json:string><json:string>Boumis et al. 2003, 2006</json:string><json:string>Peyaud et al. 2006</json:string><json:string>Morgan & Parker 1998</json:string><json:string>Acker et al. 1992, 1996</json:string><json:string>Acker et al. 1992</json:string></ref_bibl><bibl></bibl></unitex></namedEntities><ark><json:string>ark:/67375/WNG-50LL8RG4-5</json:string></ark><categories><wos><json:string>1 - science</json:string><json:string>2 - astronomy & astrophysics</json:string></wos><scienceMetrix><json:string>1 - natural sciences</json:string><json:string>2 - physics & astronomy</json:string><json:string>3 - astronomy & astrophysics</json:string></scienceMetrix><scopus><json:string>1 - Physical Sciences</json:string><json:string>2 - Earth and Planetary Sciences</json:string><json:string>3 - Space and Planetary Science</json:string><json:string>1 - Physical Sciences</json:string><json:string>2 - Physics and Astronomy</json:string><json:string>3 - Astronomy and Astrophysics</json:string></scopus><inist><json:string>1 - sciences appliquees, technologies et medecines</json:string><json:string>2 - sciences exactes et technologie</json:string><json:string>3 - terre, ocean, espace</json:string><json:string>4 - astronomie</json:string></inist></categories><publicationDate>2006</publicationDate><copyrightDate>2006</copyrightDate><doi><json:string>10.1111/j.1365-2966.2006.10950.x</json:string></doi><id>BF6D77B88884A9AF8CA9C5B5F0B6FAD2D9A8515A</id><score>1</score><fulltext><json:item><extension>pdf</extension><original>true</original><mimetype>application/pdf</mimetype><uri>https://api.istex.fr/document/BF6D77B88884A9AF8CA9C5B5F0B6FAD2D9A8515A/fulltext/pdf</uri></json:item><json:item><extension>zip</extension><original>false</original><mimetype>application/zip</mimetype><uri>https://api.istex.fr/document/BF6D77B88884A9AF8CA9C5B5F0B6FAD2D9A8515A/fulltext/zip</uri></json:item><istex:fulltextTEI uri="https://api.istex.fr/document/BF6D77B88884A9AF8CA9C5B5F0B6FAD2D9A8515A/fulltext/tei"><teiHeader><fileDesc><titleStmt><title level="a" type="main">The Macquarie/AAO/Strasbourg Hα Planetary Nebula Catalogue: MASH</title></titleStmt><publicationStmt><authority>ISTEX</authority><publisher>Blackwell Publishing Ltd</publisher><pubPlace>Oxford, UK</pubPlace><date type="published" when="2006-11-21"></date></publicationStmt><notesStmt><note type="content-type" subtype="article" source="article" scheme="https://content-type.data.istex.fr/ark:/67375/XTP-6N5SZHKN-D">article</note><note type="publication-type" subtype="journal" scheme="https://publication-type.data.istex.fr/ark:/67375/JMC-0GLKJH51-B">journal</note></notesStmt><sourceDesc><biblStruct type="article"><analytic><title level="a" type="main">The Macquarie/AAO/Strasbourg Hα Planetary Nebula Catalogue: MASH</title><title level="a" type="short">Planetary Nebula Catalogue: MASH</title><author xml:id="author-0000" role="corresp"><persName><forename type="first">Quentin A.</forename><surname>Parker</surname></persName><affiliation>Department of Physics, Macquarie University, Sydney, NSW 2109, Australia<address><country key="AU"></country></address></affiliation><affiliation>Anglo‐Australian Observatory, Epping, NSW 1710, Australia<address><country key="AU"></country></address></affiliation><affiliation>E‐mail: qap@ics.mq.edu.au</affiliation></author><author xml:id="author-0001"><persName><forename type="first">A.</forename><surname>Acker</surname></persName><affiliation>Observatoire Astronomique, Université Louis Pasteur, 67000 Strasbourg, France<address><country key="FR"></country></address></affiliation></author><author xml:id="author-0002"><persName><forename type="first">D. J.</forename><surname>Frew</surname></persName><affiliation>Department of Physics, Macquarie University, Sydney, NSW 2109, Australia<address><country key="AU"></country></address></affiliation></author><author xml:id="author-0003"><persName><forename type="first">M.</forename><surname>Hartley</surname></persName><affiliation>UK Schmidt Telescope, Anglo‐Australian Observatory, Siding Spring, 2357 NSW, Australia<address><country key="AU"></country></address></affiliation></author><author xml:id="author-0004"><persName><forename type="first">A. E. J.</forename><surname>Peyaud</surname></persName><affiliation>Department of Physics, Macquarie University, Sydney, NSW 2109, Australia<address><country key="AU"></country></address></affiliation><affiliation>Observatoire Astronomique, Université Louis Pasteur, 67000 Strasbourg, France<address><country key="FR"></country></address></affiliation></author><author xml:id="author-0005"><persName><forename type="first">F.</forename><surname>Ochsenbein</surname></persName><affiliation>Observatoire Astronomique, Université Louis Pasteur, 67000 Strasbourg, France<address><country key="FR"></country></address></affiliation></author><author xml:id="author-0006"><persName><forename type="first">S.</forename><surname>Phillipps</surname></persName><affiliation>Astrophysics Group, University of Bristol, Tyndall Avenue, Bristol BS8 1TL</affiliation></author><author xml:id="author-0007"><persName><forename type="first">D.</forename><surname>Russeil</surname></persName><affiliation>Laboratoire d'Astrophysique de Marseille, 2 Place Le Verrier, 13248 Marseille Cedex 04, France<address><country key="FR"></country></address></affiliation></author><author xml:id="author-0008"><persName><forename type="first">S. F.</forename><surname>Beaulieu</surname></persName><affiliation>Département de Physique, et Observatoire du mont Mégantic, Université Laval, Québec, QC, Canada G1K 7P4<address><country key="CA"></country></address></affiliation></author><author xml:id="author-0009"><persName><forename type="first">M.</forename><surname>Cohen</surname></persName><affiliation>Radio Astronomy Laboratory, University of California, Berkeley, CA 94720, USA<address><country key="US"></country></address></affiliation></author><author xml:id="author-0010"><persName><forename type="first">J.</forename><surname>Köppen</surname></persName><affiliation>Observatoire Astronomique, Université Louis Pasteur, 67000 Strasbourg, France<address><country key="FR"></country></address></affiliation></author><author xml:id="author-0011"><persName><forename type="first">B.</forename><surname>Miszalski</surname></persName><affiliation>Department of Physics, Macquarie University, Sydney, NSW 2109, Australia<address><country key="AU"></country></address></affiliation></author><author xml:id="author-0012"><persName><forename type="first">D. H.</forename><surname>Morgan</surname></persName><affiliation>Institute for Astronomy, School of Physics, University of Edinburgh, Edinburgh EH8 3HJ</affiliation></author><author xml:id="author-0013"><persName><forename type="first">R. A. H.</forename><surname>Morris</surname></persName><affiliation>Astrophysics Group, University of Bristol, Tyndall Avenue, Bristol BS8 1TL</affiliation></author><author xml:id="author-0014"><persName><forename type="first">M. J.</forename><surname>Pierce</surname></persName><affiliation>Department of Physics, Macquarie University, Sydney, NSW 2109, Australia<address><country key="AU"></country></address></affiliation><affiliation>Astrophysics Group, University of Bristol, Tyndall Avenue, Bristol BS8 1TL</affiliation></author><author xml:id="author-0015"><persName><forename type="first">A. E.</forename><surname>Vaughan</surname></persName><affiliation>Department of Physics, Macquarie University, Sydney, NSW 2109, Australia<address><country key="AU"></country></address></affiliation></author><idno type="istex">BF6D77B88884A9AF8CA9C5B5F0B6FAD2D9A8515A</idno><idno type="ark">ark:/67375/WNG-50LL8RG4-5</idno><idno type="DOI">10.1111/j.1365-2966.2006.10950.x</idno><idno type="unit">MNR10950</idno><idno type="toTypesetVersion">file:MNR.MNR10950.pdf</idno></analytic><monogr><title level="j" type="main">Monthly Notices of the Royal Astronomical Society</title><title level="j" type="alt">MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY</title><idno type="pISSN">0035-8711</idno><idno type="eISSN">1365-2966</idno><idno type="book-DOI">10.1111/(ISSN)1365-2966</idno><idno type="book-part-DOI">10.1111/mnr.2006.373.issue-1</idno><idno type="product">MNR</idno><idno type="publisherDivision">ST</idno><imprint><biblScope unit="vol">373</biblScope><biblScope unit="issue">1</biblScope><biblScope unit="page" from="79">79</biblScope><biblScope unit="page" to="94">94</biblScope><biblScope unit="page-count">16</biblScope><publisher>Blackwell Publishing Ltd</publisher><pubPlace>Oxford, UK</pubPlace><date type="published" when="2006-11-21"></date></imprint></monogr></biblStruct></sourceDesc></fileDesc><profileDesc><abstract xml:lang="en" style="main"><head>ABSTRACT</head><p>We present the Macquarie/AAO/Strasbourg Hα Planetary Nebula Catalogue (MASH) of over 900 true, likely and possible new Galactic planetary nebulae (PNe) discovered from the AAO/UKST Hα survey of the southern Galactic plane. The combination of depth, resolution, uniformity and areal coverage of the Hα survey has opened up a hitherto unexplored region of parameter space permitting the detection of this significant new PN sample. Away from the Galactic bulge the new PNe are typically more evolved, of larger angular extent, of lower surface brightness and more obscured (i.e. extinguished) than those in most previous surveys. We have also doubled the number of PNe in the Galactic bulge itself and although most are compact, we have also found more evolved examples. The MASH catalogue represents the culmination of a seven‐year programme of identification and confirmatory spectroscopy. A key strength is that the entire sample has been derived from the same, uniform observational data. The 60 per cent increase in known Galactic PNe represents the largest ever incremental sample of such discoveries and will have a significant impact on many aspects of PN research. This is especially important for studies at the faint end of the PN luminosity function which was previously poorly represented.</p></abstract><textClass><keywords xml:lang="en"><term xml:id="k1">astronomical data bases: miscellaneous</term><term xml:id="k2">catalogues</term><term xml:id="k3">surveys</term><term xml:id="k4">planetary nebulae: general</term></keywords><keywords rend="tocHeading1"><term>Papers</term></keywords></textClass><langUsage><language ident="en"></language></langUsage></profileDesc></teiHeader></istex:fulltextTEI><json:item><extension>txt</extension><original>false</original><mimetype>text/plain</mimetype><uri>https://api.istex.fr/document/BF6D77B88884A9AF8CA9C5B5F0B6FAD2D9A8515A/fulltext/txt</uri></json:item></fulltext><metadata><istex:metadataXml wicri:clean="Wiley, elements deleted: body"><istex:xmlDeclaration>version="1.0" encoding="UTF-8" standalone="yes"</istex:xmlDeclaration><istex:document><component version="2.0" type="serialArticle" xml:lang="en"><header><publicationMeta level="product"><publisherInfo><publisherName>Blackwell Publishing Ltd</publisherName><publisherLoc>Oxford, UK</publisherLoc></publisherInfo><doi origin="wiley" registered="yes">10.1111/(ISSN)1365-2966</doi><issn type="print">0035-8711</issn><issn type="electronic">1365-2966</issn><idGroup><id type="product" value="MNR"></id><id type="publisherDivision" value="ST"></id></idGroup><titleGroup><title type="main" sort="MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY">Monthly Notices of the Royal Astronomical Society</title></titleGroup></publicationMeta><publicationMeta level="part" position="11001"><doi origin="wiley">10.1111/mnr.2006.373.issue-1</doi><numberingGroup><numbering type="journalVolume" number="373">373</numbering><numbering type="journalIssue" number="1">1</numbering></numberingGroup><coverDate startDate="2006-11-21">November 2006</coverDate></publicationMeta><publicationMeta level="unit" type="article" position="7" status="forIssue"><doi origin="wiley">10.1111/j.1365-2966.2006.10950.x</doi><idGroup><id type="unit" value="MNR10950"></id></idGroup><countGroup><count type="pageTotal" number="16"></count></countGroup><titleGroup><title type="tocHeading1">Papers</title></titleGroup><eventGroup><event type="firstOnline" date="2006-10-25"></event><event type="publishedOnlineFinalForm" date="2006-10-25"></event><event type="xmlConverted" agent="Converter:BPG_TO_WML3G version:2.3.6 mode:FullText source:FullText result:FullText" date="2010-04-21"></event><event type="xmlConverted" agent="Converter:WILEY_ML3G_TO_WILEY_ML3GV2 version:3.8.8" date="2014-02-02"></event><event type="xmlConverted" agent="Converter:WML3G_To_WML3G version:4.1.7 mode:FullText,remove_FC" date="2014-10-31"></event></eventGroup><numberingGroup><numbering type="pageFirst" number="79">79</numbering><numbering type="pageLast" number="94">94</numbering></numberingGroup><correspondenceTo>
E‐mail: <email>qap@ics.mq.edu.au</email></correspondenceTo><linkGroup><link type="toTypesetVersion" href="file:MNR.MNR10950.pdf"></link></linkGroup></publicationMeta><contentMeta><unparsedEditorialHistory>Accepted 2006 August 15. Received 2006 August 4</unparsedEditorialHistory><countGroup><count type="figureTotal" number="8"></count><count type="tableTotal" number="2"></count><count type="formulaTotal" number="45"></count><count type="referenceTotal" number="103"></count><count type="linksCrossRef" number="177"></count></countGroup><titleGroup><title type="main">The Macquarie/AAO/Strasbourg Hα Planetary Nebula Catalogue: MASH</title><title type="shortAuthors"><i>Q. A. Parker et al.</i></title><title type="short"><i>Planetary Nebula Catalogue: MASH</i></title></titleGroup><creators><creator creatorRole="author" xml:id="cr1" affiliationRef="#a1 #a2" corresponding="yes"><personName><givenNames>Quentin A.</givenNames><familyName>Parker</familyName></personName></creator><creator creatorRole="author" xml:id="cr2" affiliationRef="#a3"><personName><givenNames>A.</givenNames><familyName>Acker</familyName></personName></creator><creator creatorRole="author" xml:id="cr3" affiliationRef="#a1"><personName><givenNames>D. J.</givenNames><familyName>Frew</familyName></personName></creator><creator creatorRole="author" xml:id="cr4" affiliationRef="#a4"><personName><givenNames>M.</givenNames><familyName>Hartley</familyName></personName></creator><creator creatorRole="author" xml:id="cr5" affiliationRef="#a1 #a3"><personName><givenNames>A. E. J.</givenNames><familyName>Peyaud</familyName></personName></creator><creator creatorRole="author" xml:id="cr6" affiliationRef="#a3"><personName><givenNames>F.</givenNames><familyName>Ochsenbein</familyName></personName></creator><creator creatorRole="author" xml:id="cr7" affiliationRef="#a5"><personName><givenNames>S.</givenNames><familyName>Phillipps</familyName></personName></creator><creator creatorRole="author" xml:id="cr8" affiliationRef="#a6"><personName><givenNames>D.</givenNames><familyName>Russeil</familyName></personName></creator><creator creatorRole="author" xml:id="cr9" affiliationRef="#a7"><personName><givenNames>S. F.</givenNames><familyName>Beaulieu</familyName></personName></creator><creator creatorRole="author" xml:id="cr10" affiliationRef="#a8"><personName><givenNames>M.</givenNames><familyName>Cohen</familyName></personName></creator><creator creatorRole="author" xml:id="cr11" affiliationRef="#a3"><personName><givenNames>J.</givenNames><familyName>Köppen</familyName></personName></creator><creator creatorRole="author" xml:id="cr12" affiliationRef="#a1"><personName><givenNames>B.</givenNames><familyName>Miszalski</familyName></personName></creator><creator creatorRole="author" xml:id="cr13" affiliationRef="#a9"><personName><givenNames>D. H.</givenNames><familyName>Morgan</familyName></personName></creator><creator creatorRole="author" xml:id="cr14" affiliationRef="#a5"><personName><givenNames>R. A. H.</givenNames><familyName>Morris</familyName></personName></creator><creator creatorRole="author" xml:id="cr15" affiliationRef="#a1 #a5"><personName><givenNames>M. J.</givenNames><familyName>Pierce</familyName></personName></creator><creator creatorRole="author" xml:id="cr16" affiliationRef="#a1"><personName><givenNames>A. E.</givenNames><familyName>Vaughan</familyName></personName></creator></creators><affiliationGroup><affiliation xml:id="a1" countryCode="AU"><unparsedAffiliation>Department of Physics, Macquarie University, Sydney, NSW 2109, Australia</unparsedAffiliation></affiliation><affiliation xml:id="a2" countryCode="AU"><unparsedAffiliation>Anglo‐Australian Observatory, Epping, NSW 1710, Australia</unparsedAffiliation></affiliation><affiliation xml:id="a3" countryCode="FR"><unparsedAffiliation>Observatoire Astronomique, Université Louis Pasteur, 67000 Strasbourg, France</unparsedAffiliation></affiliation><affiliation xml:id="a4" countryCode="AU"><unparsedAffiliation>UK Schmidt Telescope, Anglo‐Australian Observatory, Siding Spring, 2357 NSW, Australia</unparsedAffiliation></affiliation><affiliation xml:id="a5"><unparsedAffiliation>Astrophysics Group, University of Bristol, Tyndall Avenue, Bristol BS8 1TL</unparsedAffiliation></affiliation><affiliation xml:id="a6" countryCode="FR"><unparsedAffiliation>Laboratoire d'Astrophysique de Marseille, 2 Place Le Verrier, 13248 Marseille Cedex 04, France</unparsedAffiliation></affiliation><affiliation xml:id="a7" countryCode="CA"><unparsedAffiliation>Département de Physique, et Observatoire du mont Mégantic, Université Laval, Québec, QC, Canada G1K 7P4</unparsedAffiliation></affiliation><affiliation xml:id="a8" countryCode="US"><unparsedAffiliation>Radio Astronomy Laboratory, University of California, Berkeley, CA 94720, USA</unparsedAffiliation></affiliation><affiliation xml:id="a9"><unparsedAffiliation>Institute for Astronomy, School of Physics, University of Edinburgh, Edinburgh EH8 3HJ</unparsedAffiliation></affiliation></affiliationGroup><keywordGroup xml:lang="en"><keyword xml:id="k1">astronomical data bases: miscellaneous</keyword><keyword xml:id="k2">catalogues</keyword><keyword xml:id="k3">surveys</keyword><keyword xml:id="k4">planetary nebulae: general</keyword></keywordGroup><abstractGroup><abstract type="main" xml:lang="en"><title type="main">ABSTRACT</title><p>We present the Macquarie/AAO/Strasbourg Hα Planetary Nebula Catalogue (MASH) of over 900 true, likely and possible new Galactic planetary nebulae (PNe) discovered from the AAO/UKST Hα survey of the southern Galactic plane. The combination of depth, resolution, uniformity and areal coverage of the Hα survey has opened up a hitherto unexplored region of parameter space permitting the detection of this significant new PN sample. Away from the Galactic bulge the new PNe are typically more evolved, of larger angular extent, of lower surface brightness and more obscured (i.e. extinguished) than those in most previous surveys. We have also doubled the number of PNe in the Galactic bulge itself and although most are compact, we have also found more evolved examples. The MASH catalogue represents the culmination of a seven‐year programme of identification and confirmatory spectroscopy. A key strength is that the entire sample has been derived from the same, uniform observational data. The 60 per cent increase in known Galactic PNe represents the largest ever incremental sample of such discoveries and will have a significant impact on many aspects of PN research. This is especially important for studies at the faint end of the PN luminosity function which was previously poorly represented.</p></abstract></abstractGroup></contentMeta></header></component></istex:document></istex:metadataXml><mods version="3.6"><titleInfo lang="en"><title>The Macquarie/AAO/Strasbourg Hα Planetary Nebula Catalogue: MASH</title></titleInfo><titleInfo type="abbreviated" lang="en"><title>Planetary Nebula Catalogue: MASH</title></titleInfo><titleInfo type="alternative" contentType="CDATA" lang="en"><title>The Macquarie/AAO/Strasbourg Hα Planetary Nebula Catalogue: MASH</title></titleInfo><name type="personal"><namePart type="given">Quentin A.</namePart><namePart type="family">Parker</namePart><affiliation>Department of Physics, Macquarie University, Sydney, NSW 2109, Australia</affiliation><affiliation>Anglo‐Australian Observatory, Epping, NSW 1710, Australia</affiliation><affiliation>E-mail: qap@ics.mq.edu.au</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">A.</namePart><namePart type="family">Acker</namePart><affiliation>Observatoire Astronomique, Université Louis Pasteur, 67000 Strasbourg, France</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">D. J.</namePart><namePart type="family">Frew</namePart><affiliation>Department of Physics, Macquarie University, Sydney, NSW 2109, Australia</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">M.</namePart><namePart type="family">Hartley</namePart><affiliation>UK Schmidt Telescope, Anglo‐Australian Observatory, Siding Spring, 2357 NSW, Australia</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">A. E. J.</namePart><namePart type="family">Peyaud</namePart><affiliation>Department of Physics, Macquarie University, Sydney, NSW 2109, Australia</affiliation><affiliation>Observatoire Astronomique, Université Louis Pasteur, 67000 Strasbourg, France</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">F.</namePart><namePart type="family">Ochsenbein</namePart><affiliation>Observatoire Astronomique, Université Louis Pasteur, 67000 Strasbourg, France</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">S.</namePart><namePart type="family">Phillipps</namePart><affiliation>Astrophysics Group, University of Bristol, Tyndall Avenue, Bristol BS8 1TL</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">D.</namePart><namePart type="family">Russeil</namePart><affiliation>Laboratoire d'Astrophysique de Marseille, 2 Place Le Verrier, 13248 Marseille Cedex 04, France</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">S. F.</namePart><namePart type="family">Beaulieu</namePart><affiliation>Département de Physique, et Observatoire du mont Mégantic, Université Laval, Québec, QC, Canada G1K 7P4</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">M.</namePart><namePart type="family">Cohen</namePart><affiliation>Radio Astronomy Laboratory, University of California, Berkeley, CA 94720, USA</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">J.</namePart><namePart type="family">Köppen</namePart><affiliation>Observatoire Astronomique, Université Louis Pasteur, 67000 Strasbourg, France</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">B.</namePart><namePart type="family">Miszalski</namePart><affiliation>Department of Physics, Macquarie University, Sydney, NSW 2109, Australia</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">D. H.</namePart><namePart type="family">Morgan</namePart><affiliation>Institute for Astronomy, School of Physics, University of Edinburgh, Edinburgh EH8 3HJ</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">R. A. H.</namePart><namePart type="family">Morris</namePart><affiliation>Astrophysics Group, University of Bristol, Tyndall Avenue, Bristol BS8 1TL</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">M. J.</namePart><namePart type="family">Pierce</namePart><affiliation>Department of Physics, Macquarie University, Sydney, NSW 2109, Australia</affiliation><affiliation>Astrophysics Group, University of Bristol, Tyndall Avenue, Bristol BS8 1TL</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">A. E.</namePart><namePart type="family">Vaughan</namePart><affiliation>Department of Physics, Macquarie University, Sydney, NSW 2109, Australia</affiliation><role><roleTerm type="text">author</roleTerm></role></name><typeOfResource>text</typeOfResource><genre type="article" displayLabel="article" authority="ISTEX" authorityURI="https://content-type.data.istex.fr" valueURI="https://content-type.data.istex.fr/ark:/67375/XTP-6N5SZHKN-D">article</genre><originInfo><publisher>Blackwell Publishing Ltd</publisher><place><placeTerm type="text">Oxford, UK</placeTerm></place><dateIssued encoding="w3cdtf">2006-11-21</dateIssued><edition>Accepted 2006 August 15. Received 2006 August 4</edition><copyrightDate encoding="w3cdtf">2006</copyrightDate></originInfo><language><languageTerm type="code" authority="rfc3066">en</languageTerm><languageTerm type="code" authority="iso639-2b">eng</languageTerm></language><physicalDescription><extent unit="figures">8</extent><extent unit="tables">2</extent><extent unit="formulas">45</extent><extent unit="references">103</extent><extent unit="linksCrossRef">177</extent></physicalDescription><abstract lang="en">We present the Macquarie/AAO/Strasbourg Hα Planetary Nebula Catalogue (MASH) of over 900 true, likely and possible new Galactic planetary nebulae (PNe) discovered from the AAO/UKST Hα survey of the southern Galactic plane. The combination of depth, resolution, uniformity and areal coverage of the Hα survey has opened up a hitherto unexplored region of parameter space permitting the detection of this significant new PN sample. Away from the Galactic bulge the new PNe are typically more evolved, of larger angular extent, of lower surface brightness and more obscured (i.e. extinguished) than those in most previous surveys. We have also doubled the number of PNe in the Galactic bulge itself and although most are compact, we have also found more evolved examples. The MASH catalogue represents the culmination of a seven‐year programme of identification and confirmatory spectroscopy. A key strength is that the entire sample has been derived from the same, uniform observational data. The 60 per cent increase in known Galactic PNe represents the largest ever incremental sample of such discoveries and will have a significant impact on many aspects of PN research. This is especially important for studies at the faint end of the PN luminosity function which was previously poorly represented.</abstract><subject lang="en"><genre>keywords</genre><topic>astronomical data bases: miscellaneous</topic><topic>catalogues</topic><topic>surveys</topic><topic>planetary nebulae: general</topic></subject><relatedItem type="host"><titleInfo><title>Monthly Notices of the Royal Astronomical Society</title></titleInfo><genre type="journal" authority="ISTEX" authorityURI="https://publication-type.data.istex.fr" valueURI="https://publication-type.data.istex.fr/ark:/67375/JMC-0GLKJH51-B">journal</genre><identifier type="ISSN">0035-8711</identifier><identifier type="eISSN">1365-2966</identifier><identifier type="DOI">10.1111/(ISSN)1365-2966</identifier><identifier type="PublisherID">MNR</identifier><part><date>2006</date><detail type="volume"><caption>vol.</caption><number>373</number></detail><detail type="issue"><caption>no.</caption><number>1</number></detail><extent unit="pages"><start>79</start><end>94</end><total>16</total></extent></part></relatedItem><identifier type="istex">BF6D77B88884A9AF8CA9C5B5F0B6FAD2D9A8515A</identifier><identifier type="ark">ark:/67375/WNG-50LL8RG4-5</identifier><identifier type="DOI">10.1111/j.1365-2966.2006.10950.x</identifier><identifier type="ArticleID">MNR10950</identifier><recordInfo><recordContentSource authority="ISTEX" authorityURI="https://loaded-corpus.data.istex.fr" valueURI="https://loaded-corpus.data.istex.fr/ark:/67375/XBH-L0C46X92-X">wiley</recordContentSource><recordOrigin>Blackwell Publishing Ltd</recordOrigin></recordInfo></mods><json:item><extension>json</extension><original>false</original><mimetype>application/json</mimetype><uri>https://api.istex.fr/document/BF6D77B88884A9AF8CA9C5B5F0B6FAD2D9A8515A/metadata/json</uri></json:item></metadata><serie></serie></istex></record>Pour manipuler ce document sous Unix (Dilib)
EXPLOR_STEP=$WICRI_ROOT/Wicri/Asie/explor/AustralieFrV1/Data/Istex/Corpus
HfdSelect -h $EXPLOR_STEP/biblio.hfd -nk 002366 | SxmlIndent | more
Ou
HfdSelect -h $EXPLOR_AREA/Data/Istex/Corpus/biblio.hfd -nk 002366 | SxmlIndent | more
Pour mettre un lien sur cette page dans le réseau Wicri
{{Explor lien
|wiki= Wicri/Asie
|area= AustralieFrV1
|flux= Istex
|étape= Corpus
|type= RBID
|clé= ISTEX:BF6D77B88884A9AF8CA9C5B5F0B6FAD2D9A8515A
|texte= The Macquarie/AAO/Strasbourg Hα Planetary Nebula Catalogue: MASH
}}
| This area was generated with Dilib version V0.6.33. |  |