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The Macquarie/AAO/Strasbourg Hα Planetary Nebula Catalogue: MASH

Identifieur interne : 009886 ( Main/Exploration ); précédent : 009885; suivant : 009887

The Macquarie/AAO/Strasbourg Hα Planetary Nebula Catalogue: MASH

Auteurs : Quentin A. Parker [Australie] ; A. Acker [France] ; D. J. Frew [Australie] ; M. Hartley [Australie] ; A. E. J. Peyaud [Australie, France] ; F. Ochsenbein [France] ; S. Phillipps ; D. Russeil [France] ; S. F. Beaulieu [Canada] ; M. Cohen [États-Unis] ; J. Köppen [France] ; B. Miszalski [Australie] ; D. H. Morgan [Royaume-Uni] ; R. A. H. Morris ; M. J. Pierce [Australie] ; A. E. Vaughan [Australie]

Source :

RBID : ISTEX:BF6D77B88884A9AF8CA9C5B5F0B6FAD2D9A8515A

Descripteurs français

English descriptors

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


Affiliations:


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Le document en format XML

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<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="Wicri" type="topic" xml:lang="fr">
<term>Catalogue</term>
<term>Spectrométrie</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>
<affiliations>
<list>
<country>
<li>Australie</li>
<li>Canada</li>
<li>France</li>
<li>Royaume-Uni</li>
<li>États-Unis</li>
</country>
<region>
<li>Alsace (région administrative)</li>
<li>Californie</li>
<li>Grand Est</li>
<li>Écosse</li>
</region>
<settlement>
<li>Strasbourg</li>
<li>Édimbourg</li>
</settlement>
<orgName>
<li>Université Strasbourg 1</li>
<li>Université d'Édimbourg</li>
</orgName>
</list>
<tree>
<noCountry>
<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>
<name sortKey="Phillipps, S" sort="Phillipps, S" uniqKey="Phillipps S" first="S." last="Phillipps">S. Phillipps</name>
</noCountry>
<country name="Australie">
<noRegion>
<name sortKey="Parker, Quentin A" sort="Parker, Quentin A" uniqKey="Parker Q" first="Quentin A." last="Parker">Quentin A. Parker</name>
</noRegion>
<name sortKey="Frew, D J" sort="Frew, D J" uniqKey="Frew D" first="D. J." last="Frew">D. J. Frew</name>
<name sortKey="Hartley, M" sort="Hartley, M" uniqKey="Hartley M" first="M." last="Hartley">M. Hartley</name>
<name sortKey="Miszalski, B" sort="Miszalski, B" uniqKey="Miszalski B" first="B." last="Miszalski">B. Miszalski</name>
<name sortKey="Parker, Quentin A" sort="Parker, Quentin A" uniqKey="Parker Q" first="Quentin A." last="Parker">Quentin A. Parker</name>
<name sortKey="Parker, Quentin A" sort="Parker, Quentin A" uniqKey="Parker Q" first="Quentin A." last="Parker">Quentin A. Parker</name>
<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>
<name sortKey="Pierce, M J" sort="Pierce, M J" uniqKey="Pierce M" first="M. J." last="Pierce">M. J. Pierce</name>
<name sortKey="Vaughan, A E" sort="Vaughan, A E" uniqKey="Vaughan A" first="A. E." last="Vaughan">A. E. Vaughan</name>
</country>
<country name="France">
<region name="Grand Est">
<name sortKey="Acker, A" sort="Acker, A" uniqKey="Acker A" first="A." last="Acker">A. Acker</name>
</region>
<name sortKey="Koppen, J" sort="Koppen, J" uniqKey="Koppen J" first="J." last="Köppen">J. Köppen</name>
<name sortKey="Ochsenbein, F" sort="Ochsenbein, F" uniqKey="Ochsenbein F" first="F." last="Ochsenbein">F. Ochsenbein</name>
<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>
<name sortKey="Russeil, D" sort="Russeil, D" uniqKey="Russeil D" first="D." last="Russeil">D. Russeil</name>
</country>
<country name="Canada">
<noRegion>
<name sortKey="Beaulieu, S F" sort="Beaulieu, S F" uniqKey="Beaulieu S" first="S. F." last="Beaulieu">S. F. Beaulieu</name>
</noRegion>
</country>
<country name="États-Unis">
<region name="Californie">
<name sortKey="Cohen, M" sort="Cohen, M" uniqKey="Cohen M" first="M." last="Cohen">M. Cohen</name>
</region>
</country>
<country name="Royaume-Uni">
<region name="Écosse">
<name sortKey="Morgan, D H" sort="Morgan, D H" uniqKey="Morgan D" first="D. H." last="Morgan">D. H. Morgan</name>
</region>
</country>
</tree>
</affiliations>
</record>

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