Multisite campaign on the open cluster M67 – III. δ Scuti pulsations in the blue stragglers
Identifieur interne : 009122 ( Main/Exploration ); précédent : 009121; suivant : 009123Multisite campaign on the open cluster M67 – III. δ Scuti pulsations in the blue stragglers
Auteurs : H. Bruntt [Australie] ; D. Stello [Australie, Danemark, États-Unis] ; J. C. Suárez [Espagne, France] ; T. Arentoft [Danemark] ; T. R. Bedding [Australie] ; M. Y. Bouzid [Belgique] ; Z. Csubry [Hongrie] ; T. H. Dall [États-Unis, Chili] ; Z. E. Dind [Australie] ; S. Frandsen [Danemark] ; R. L. Gilliland [États-Unis] ; A. P. Jacob [Australie] ; H. R. Jensen [Danemark] ; Y. B. Kang [Corée du Sud] ; S. Kim [Corée du Sud] ; L. L. Kiss [Australie] ; H. Kjeldsen [Danemark] ; J. Koo [Corée du Sud] ; J. Lee [Corée du Sud] ; C. Lee [Corée du Sud] ; J. Nuspl [Hongrie] ; C. Sterken [Belgique] ; R. Szab [Hongrie, États-Unis]Source :
- Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 2007-07-11.
Descripteurs français
- Pascal (Inist)
- Wicri :
- topic : Niveau sonore, Simulation, Spectrométrie.
English descriptors
- KwdEn :
- Alias, Amplitude, Amplitude ratios, Amplitude spectra, Amplitude spectrum, Asteroseismic analysis, Astronomy observatory, Autocorrelation, Autocorrelations, Average scatter, Binary stars, Blue stragglers, Bottom panel, Bottom panels, Breger, Bruntt, Comb pattern, Complete light curve, Correlation length, Current data, Daejeon korea, Data point, Data points, Delta Scuti stars, Detectable amplitudes, Different calibrations, Different symbols, Dominant modes, Dominant peak, Drift noise, Dziembowski, Fourier analysis, Frequency, Frequency range, Fundamental parameters, General agreement, Gilliland, Globular clusters, Goupil houdek, Gradual coalescence, Grey squares, Grid, High mass, Histogram, Horizontal bars, Horizontal line marks, Insets show, Instability strip, Journal compilation, Kitt peak, Korea astronomy, Large number, Large separation, Last column, Light curve, Light curves, Linear combinations, Lled, Lled circles, Lled symbols, Loao, Lower amplitude peaks, Lowest noise level, Lter, Lter data, Many cases, Middle panel, Mmag, Mnras, Model grid, Models, N color photometry, Neighbouring data points, Noise level, Noise levels, Open cluster, Open clusters, Oscillation, Oscillation frequencies, Other scuti stars, Other stars, Outlier, Outlier weight, Outlier weights, Outlier weights wout, Photometric, Photometric error boxes, Pulsation, Pulsation frequencies, Pulsation models, Radial modes, Reference star, Reference stars, Regular pattern, Relative amplitudes, Residual spectra, Residual spectrum, Rotational splitting, Rotational velocities, Sander, Sandquist shetrone, Scatter, Scatter weight, Scatter weights, Scatter weights wscat, Scuti, Scuti pulsations, Scuti star, Scuti stars, Simulation, Space science institute, Spectral window, Spectral windows, Spectroscopy, Star, Star clusters, Stellar, Straggler, Target star, Teff, Theoretical frequencies, Theoretical models, Theoretical pulsation models, Time series, Typical scatter, Uncorrelated noise, Vertical lines, Weaker frequencies, White noise, Wout, Wscat.
- Teeft :
- Alias, Amplitude, Amplitude ratios, Amplitude spectra, Amplitude spectrum, Asteroseismic analysis, Astronomy observatory, Autocorrelation, Autocorrelations, Average scatter, Binary stars, Blue stragglers, Bottom panel, Bottom panels, Breger, Bruntt, Comb pattern, Complete light curve, Correlation length, Current data, Daejeon korea, Data point, Data points, Detectable amplitudes, Different calibrations, Different symbols, Dominant modes, Dominant peak, Drift noise, Dziembowski, Fourier analysis, Frequency, Frequency range, Fundamental parameters, General agreement, Gilliland, Globular clusters, Goupil houdek, Gradual coalescence, Grey squares, Grid, High mass, Histogram, Horizontal bars, Horizontal line marks, Insets show, Instability strip, Journal compilation, Kitt peak, Korea astronomy, Large number, Large separation, Last column, Light curve, Light curves, Linear combinations, Lled, Lled circles, Lled symbols, Loao, Lower amplitude peaks, Lowest noise level, Lter, Lter data, Many cases, Middle panel, Mmag, Mnras, Model grid, Neighbouring data points, Noise level, Noise levels, Open cluster, Open clusters, Oscillation, Oscillation frequencies, Other scuti stars, Other stars, Outlier, Outlier weight, Outlier weights, Outlier weights wout, Photometric, Photometric error boxes, Pulsation, Pulsation frequencies, Pulsation models, Radial modes, Reference star, Reference stars, Regular pattern, Relative amplitudes, Residual spectra, Residual spectrum, Rotational splitting, Rotational velocities, Sander, Sandquist shetrone, Scatter, Scatter weight, Scatter weights, Scatter weights wscat, Scuti, Scuti pulsations, Scuti star, Scuti stars, Simulation, Space science institute, Spectral window, Spectral windows, Star, Stellar, Straggler, Target star, Teff, Theoretical frequencies, Theoretical models, Theoretical pulsation models, Typical scatter, Uncorrelated noise, Vertical lines, Weaker frequencies, White noise, Wout, Wscat.
Abstract
We have made an asteroseismic analysis of the variable blue stragglers in the open cluster M67. The data set consists of photometric time‐series from eight sites using nine 0.6–2.1 m telescopes with a time‐baseline of 43 d. In two stars, EW Cnc and EX Cnc, we detect the highest number of frequencies (41 and 26) detected in δ Scuti stars belonging to a stellar cluster, and EW Cnc has the second highest number of frequencies detected in any δ Scuti star. We have computed a grid of pulsation models that take the effects of rotation into account. The distribution of observed and theoretical frequencies shows that in a wide frequency range a significant fraction of the radial and non‐radial low‐degree modes are excited to detectable amplitudes. Despite the large number of observed frequencies we cannot constrain the fundamental parameters of the stars. To make progress we need to identify the degrees of some of the modes from either multicolour photometry or spectroscopy.
Url:
- https://api.istex.fr/document/E314D55C11BF66413069810356782E82066B0662/fulltext/pdf
- https://api.istex.fr/document/6C0F9E5242653A4EEC830E13AC9B1C085EFEC08E/fulltext/pdf
DOI: 10.1111/j.1365-2966.2007.11865.x
Affiliations:
- Australie, Belgique, Chili, Corée du Sud, Danemark, Espagne, France, Hongrie, États-Unis
- Colorado, Floride, Hawaï, Maryland, Nouvelle-Galles du Sud
- Baltimore, Sydney
- Université de Sydney
Links toward previous steps (curation, corpus...)
- to stream Istex, to step Corpus: 002A61
- to stream Istex, to step Curation: 002A61
- to stream Istex, to step Checkpoint: 001371
- to stream Istex, to step Corpus: 001423
- to stream Istex, to step Curation: 001423
- to stream Istex, to step Checkpoint: 001297
- to stream Main, to step Merge: 009A95
- to stream PascalFrancis, to step Corpus: 003B36
- to stream PascalFrancis, to step Curation: 002552
- to stream PascalFrancis, to step Checkpoint: 003760
- to stream Main, to step Merge: 009E72
- to stream Main, to step Curation: 009122
Le document en format XML
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Csubry</name><affiliation wicri:level="1"><country xml:lang="fr">Hongrie</country><wicri:regionArea>Konkoly Observatory of the Hungarian Academy of Sciences, H‐1525 Budapest, PO Box 67</wicri:regionArea><wicri:noRegion>PO Box 67</wicri:noRegion></affiliation></author><author><name sortKey="Dall, T H" sort="Dall, T H" uniqKey="Dall T" first="T. H." last="Dall">T. H. Dall</name><affiliation wicri:level="2"><country xml:lang="fr">États-Unis</country><wicri:regionArea>Gemini Observatory, 670 N. A'ohoku Pl., Hilo, HI 96720</wicri:regionArea><placeName><region type="state">Hawaï</region></placeName></affiliation><affiliation wicri:level="1"><country xml:lang="fr">Chili</country><wicri:regionArea>European Southern Observatory, Casilla 19001, Santiago 19</wicri:regionArea><wicri:noRegion>Santiago 19</wicri:noRegion></affiliation></author><author><name sortKey="Dind, Z E" sort="Dind, Z E" uniqKey="Dind Z" first="Z. E." last="Dind">Z. E. 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Frandsen</name><affiliation wicri:level="1"><country xml:lang="fr">Danemark</country><wicri:regionArea>Institut for Fysik og Astronomi (IFA), University of Aarhus, DK‐8000 Aarhus</wicri:regionArea><wicri:noRegion>DK‐8000 Aarhus</wicri:noRegion></affiliation><affiliation wicri:level="1"><country xml:lang="fr">Danemark</country><wicri:regionArea>Danish AsteroSeismology Centre, University of Aarhus, DK‐8000 Aarhus</wicri:regionArea><wicri:noRegion>DK‐8000 Aarhus</wicri:noRegion></affiliation></author><author><name sortKey="Gilliland, R L" sort="Gilliland, R L" uniqKey="Gilliland R" first="R. L." last="Gilliland">R. L. 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Jensen</name><affiliation wicri:level="1"><country xml:lang="fr">Danemark</country><wicri:regionArea>Institut for Fysik og Astronomi (IFA), University of Aarhus, DK‐8000 Aarhus</wicri:regionArea><wicri:noRegion>DK‐8000 Aarhus</wicri:noRegion></affiliation></author><author><name sortKey="Kang, Y B" sort="Kang, Y B" uniqKey="Kang Y" first="Y. B." last="Kang">Y. B. Kang</name><affiliation wicri:level="1"><country xml:lang="fr">Corée du Sud</country><wicri:regionArea>Department of Astronomy and Space Science, Chungnam National University, Daejeon 305‐764</wicri:regionArea><wicri:noRegion>Daejeon 305‐764</wicri:noRegion></affiliation></author><author><name sortKey="Kim, S" sort="Kim, S" uniqKey="Kim S" first="S." last="Kim">S. Kim</name><affiliation wicri:level="1"><country xml:lang="fr">Corée du Sud</country><wicri:regionArea>Korea Astronomy and Space Science Institute, Daejeon 305‐348</wicri:regionArea><wicri:noRegion>Daejeon 305‐348</wicri:noRegion></affiliation></author><author><name sortKey="Kiss, L L" sort="Kiss, L L" uniqKey="Kiss L" first="L. L." last="Kiss">L. L. Kiss</name><affiliation wicri:level="4"><country xml:lang="fr">Australie</country><wicri:regionArea>School of Physics, University of Sydney, NSW 2006</wicri:regionArea><orgName type="university">Université de Sydney</orgName><placeName><settlement type="city">Sydney</settlement><region type="état">Nouvelle-Galles du Sud</region></placeName></affiliation></author><author><name sortKey="Kjeldsen, H" sort="Kjeldsen, H" uniqKey="Kjeldsen H" first="H." last="Kjeldsen">H. Kjeldsen</name><affiliation wicri:level="1"><country xml:lang="fr">Danemark</country><wicri:regionArea>Institut for Fysik og Astronomi (IFA), University of Aarhus, DK‐8000 Aarhus</wicri:regionArea><wicri:noRegion>DK‐8000 Aarhus</wicri:noRegion></affiliation><affiliation wicri:level="1"><country xml:lang="fr">Danemark</country><wicri:regionArea>Danish AsteroSeismology Centre, University of Aarhus, DK‐8000 Aarhus</wicri:regionArea><wicri:noRegion>DK‐8000 Aarhus</wicri:noRegion></affiliation></author><author><name sortKey="Koo, J" sort="Koo, J" uniqKey="Koo J" first="J." last="Koo">J. Koo</name><affiliation wicri:level="1"><country xml:lang="fr">Corée du Sud</country><wicri:regionArea>Department of Astronomy and Space Science, Chungnam National University, Daejeon 305‐764</wicri:regionArea><wicri:noRegion>Daejeon 305‐764</wicri:noRegion></affiliation></author><author><name sortKey="Lee, J" sort="Lee, J" uniqKey="Lee J" first="J." last="Lee">J. Lee</name><affiliation wicri:level="1"><country xml:lang="fr">Corée du Sud</country><wicri:regionArea>Korea Astronomy and Space Science Institute, Daejeon 305‐348</wicri:regionArea><wicri:noRegion>Daejeon 305‐348</wicri:noRegion></affiliation></author><author><name sortKey="Lee, C" sort="Lee, C" uniqKey="Lee C" first="C." last="Lee">C. Lee</name><affiliation wicri:level="1"><country xml:lang="fr">Corée du Sud</country><wicri:regionArea>Korea Astronomy and Space Science Institute, Daejeon 305‐348</wicri:regionArea><wicri:noRegion>Daejeon 305‐348</wicri:noRegion></affiliation></author><author><name sortKey="Nuspl, J" sort="Nuspl, J" uniqKey="Nuspl J" first="J." last="Nuspl">J. Nuspl</name><affiliation wicri:level="1"><country xml:lang="fr">Hongrie</country><wicri:regionArea>Konkoly Observatory of the Hungarian Academy of Sciences, H‐1525 Budapest, PO Box 67</wicri:regionArea><wicri:noRegion>PO Box 67</wicri:noRegion></affiliation></author><author><name sortKey="Sterken, C" sort="Sterken, C" uniqKey="Sterken C" first="C." last="Sterken">C. Sterken</name><affiliation wicri:level="1"><country xml:lang="fr">Belgique</country><wicri:regionArea>Vrije Universiteit Brussel, Pleinlaan 2, B‐1050 Brussels</wicri:regionArea><wicri:noRegion>B‐1050 Brussels</wicri:noRegion></affiliation></author><author><name sortKey="Szab, R" sort="Szab, R" uniqKey="Szab R" first="R." last="Szab">R. Szab</name><affiliation wicri:level="1"><country xml:lang="fr">Hongrie</country><wicri:regionArea>Konkoly Observatory of the Hungarian Academy of Sciences, H‐1525 Budapest, PO Box 67</wicri:regionArea><wicri:noRegion>PO Box 67</wicri:noRegion></affiliation><affiliation wicri:level="2"><country xml:lang="fr">États-Unis</country><wicri:regionArea>Physics Department, University of Florida, Gainesville, FL 32611</wicri:regionArea><placeName><region type="state">Floride</region></placeName></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">378</biblScope><biblScope unit="issue">4</biblScope><biblScope unit="page" from="1371">1371</biblScope><biblScope unit="page" to="1384">1384</biblScope><biblScope unit="page-count">14</biblScope><publisher>Blackwell Publishing Ltd</publisher><pubPlace>Oxford, UK</pubPlace><date type="published" when="2007-07-11">2007-07-11</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>Alias</term><term>Amplitude</term><term>Amplitude ratios</term><term>Amplitude spectra</term><term>Amplitude spectrum</term><term>Asteroseismic analysis</term><term>Astronomy observatory</term><term>Autocorrelation</term><term>Autocorrelations</term><term>Average scatter</term><term>Binary stars</term><term>Blue stragglers</term><term>Bottom panel</term><term>Bottom panels</term><term>Breger</term><term>Bruntt</term><term>Comb pattern</term><term>Complete light curve</term><term>Correlation length</term><term>Current data</term><term>Daejeon korea</term><term>Data point</term><term>Data points</term><term>Delta Scuti stars</term><term>Detectable amplitudes</term><term>Different calibrations</term><term>Different symbols</term><term>Dominant modes</term><term>Dominant peak</term><term>Drift noise</term><term>Dziembowski</term><term>Fourier analysis</term><term>Frequency</term><term>Frequency range</term><term>Fundamental parameters</term><term>General agreement</term><term>Gilliland</term><term>Globular clusters</term><term>Goupil houdek</term><term>Gradual coalescence</term><term>Grey squares</term><term>Grid</term><term>High mass</term><term>Histogram</term><term>Horizontal bars</term><term>Horizontal line marks</term><term>Insets show</term><term>Instability strip</term><term>Journal compilation</term><term>Kitt peak</term><term>Korea astronomy</term><term>Large number</term><term>Large separation</term><term>Last column</term><term>Light curve</term><term>Light curves</term><term>Linear combinations</term><term>Lled</term><term>Lled circles</term><term>Lled symbols</term><term>Loao</term><term>Lower amplitude peaks</term><term>Lowest noise level</term><term>Lter</term><term>Lter data</term><term>Many cases</term><term>Middle panel</term><term>Mmag</term><term>Mnras</term><term>Model grid</term><term>Models</term><term>N color photometry</term><term>Neighbouring data points</term><term>Noise level</term><term>Noise levels</term><term>Open cluster</term><term>Open clusters</term><term>Oscillation</term><term>Oscillation frequencies</term><term>Other scuti stars</term><term>Other stars</term><term>Outlier</term><term>Outlier weight</term><term>Outlier weights</term><term>Outlier weights wout</term><term>Photometric</term><term>Photometric error boxes</term><term>Pulsation</term><term>Pulsation frequencies</term><term>Pulsation models</term><term>Radial modes</term><term>Reference star</term><term>Reference stars</term><term>Regular pattern</term><term>Relative amplitudes</term><term>Residual spectra</term><term>Residual spectrum</term><term>Rotational splitting</term><term>Rotational velocities</term><term>Sander</term><term>Sandquist shetrone</term><term>Scatter</term><term>Scatter weight</term><term>Scatter weights</term><term>Scatter weights wscat</term><term>Scuti</term><term>Scuti pulsations</term><term>Scuti star</term><term>Scuti stars</term><term>Simulation</term><term>Space science institute</term><term>Spectral window</term><term>Spectral windows</term><term>Spectroscopy</term><term>Star</term><term>Star clusters</term><term>Stellar</term><term>Straggler</term><term>Target star</term><term>Teff</term><term>Theoretical frequencies</term><term>Theoretical models</term><term>Theoretical pulsation models</term><term>Time series</term><term>Typical scatter</term><term>Uncorrelated noise</term><term>Vertical lines</term><term>Weaker frequencies</term><term>White noise</term><term>Wout</term><term>Wscat</term></keywords><keywords scheme="Pascal" xml:lang="fr"><term>Amas ouvert</term><term>Amas stellaire</term><term>Blue straggler</term><term>Etoile type delta Scuti</term><term>Modèle</term><term>Photométrie n couleurs</term><term>Spectrométrie</term><term>Série temporelle</term></keywords><keywords scheme="Teeft" xml:lang="en"><term>Alias</term><term>Amplitude</term><term>Amplitude ratios</term><term>Amplitude spectra</term><term>Amplitude spectrum</term><term>Asteroseismic analysis</term><term>Astronomy observatory</term><term>Autocorrelation</term><term>Autocorrelations</term><term>Average scatter</term><term>Binary stars</term><term>Blue stragglers</term><term>Bottom panel</term><term>Bottom panels</term><term>Breger</term><term>Bruntt</term><term>Comb pattern</term><term>Complete light curve</term><term>Correlation length</term><term>Current data</term><term>Daejeon korea</term><term>Data point</term><term>Data points</term><term>Detectable amplitudes</term><term>Different calibrations</term><term>Different symbols</term><term>Dominant modes</term><term>Dominant peak</term><term>Drift noise</term><term>Dziembowski</term><term>Fourier analysis</term><term>Frequency</term><term>Frequency range</term><term>Fundamental parameters</term><term>General agreement</term><term>Gilliland</term><term>Globular clusters</term><term>Goupil houdek</term><term>Gradual coalescence</term><term>Grey squares</term><term>Grid</term><term>High mass</term><term>Histogram</term><term>Horizontal bars</term><term>Horizontal line marks</term><term>Insets show</term><term>Instability strip</term><term>Journal compilation</term><term>Kitt peak</term><term>Korea astronomy</term><term>Large number</term><term>Large separation</term><term>Last column</term><term>Light curve</term><term>Light curves</term><term>Linear combinations</term><term>Lled</term><term>Lled circles</term><term>Lled symbols</term><term>Loao</term><term>Lower amplitude peaks</term><term>Lowest noise level</term><term>Lter</term><term>Lter data</term><term>Many cases</term><term>Middle panel</term><term>Mmag</term><term>Mnras</term><term>Model grid</term><term>Neighbouring data points</term><term>Noise level</term><term>Noise levels</term><term>Open cluster</term><term>Open clusters</term><term>Oscillation</term><term>Oscillation frequencies</term><term>Other scuti stars</term><term>Other stars</term><term>Outlier</term><term>Outlier weight</term><term>Outlier weights</term><term>Outlier weights wout</term><term>Photometric</term><term>Photometric error boxes</term><term>Pulsation</term><term>Pulsation frequencies</term><term>Pulsation models</term><term>Radial modes</term><term>Reference star</term><term>Reference stars</term><term>Regular pattern</term><term>Relative amplitudes</term><term>Residual spectra</term><term>Residual spectrum</term><term>Rotational splitting</term><term>Rotational velocities</term><term>Sander</term><term>Sandquist shetrone</term><term>Scatter</term><term>Scatter weight</term><term>Scatter weights</term><term>Scatter weights wscat</term><term>Scuti</term><term>Scuti pulsations</term><term>Scuti star</term><term>Scuti stars</term><term>Simulation</term><term>Space science institute</term><term>Spectral window</term><term>Spectral windows</term><term>Star</term><term>Stellar</term><term>Straggler</term><term>Target star</term><term>Teff</term><term>Theoretical frequencies</term><term>Theoretical models</term><term>Theoretical pulsation models</term><term>Typical scatter</term><term>Uncorrelated noise</term><term>Vertical lines</term><term>Weaker frequencies</term><term>White noise</term><term>Wout</term><term>Wscat</term></keywords><keywords scheme="Wicri" type="topic" xml:lang="fr"><term>Niveau sonore</term><term>Simulation</term><term>Spectrométrie</term></keywords></textClass></profileDesc></teiHeader><front><div type="abstract" xml:lang="en">We have made an asteroseismic analysis of the variable blue stragglers in the open cluster M67. The data set consists of photometric time‐series from eight sites using nine 0.6–2.1 m telescopes with a time‐baseline of 43 d. In two stars, EW Cnc and EX Cnc, we detect the highest number of frequencies (41 and 26) detected in δ Scuti stars belonging to a stellar cluster, and EW Cnc has the second highest number of frequencies detected in any δ Scuti star. We have computed a grid of pulsation models that take the effects of rotation into account. The distribution of observed and theoretical frequencies shows that in a wide frequency range a significant fraction of the radial and non‐radial low‐degree modes are excited to detectable amplitudes. Despite the large number of observed frequencies we cannot constrain the fundamental parameters of the stars. To make progress we need to identify the degrees of some of the modes from either multicolour photometry or spectroscopy.</div></front></TEI><affiliations><list><country><li>Australie</li><li>Belgique</li><li>Chili</li><li>Corée du Sud</li><li>Danemark</li><li>Espagne</li><li>France</li><li>Hongrie</li><li>États-Unis</li></country><region><li>Colorado</li><li>Floride</li><li>Hawaï</li><li>Maryland</li><li>Nouvelle-Galles du Sud</li></region><settlement><li>Baltimore</li><li>Sydney</li></settlement><orgName><li>Université de Sydney</li></orgName></list><tree><country name="Australie"><region name="Nouvelle-Galles du Sud"><name sortKey="Bruntt, H" sort="Bruntt, H" uniqKey="Bruntt H" first="H." last="Bruntt">H. Bruntt</name></region><name sortKey="Bedding, T R" sort="Bedding, T R" uniqKey="Bedding T" first="T. R." last="Bedding">T. R. Bedding</name><name sortKey="Bruntt, H" sort="Bruntt, H" uniqKey="Bruntt H" first="H." last="Bruntt">H. Bruntt</name><name sortKey="Dind, Z E" sort="Dind, Z E" uniqKey="Dind Z" first="Z. E." last="Dind">Z. E. Dind</name><name sortKey="Jacob, A P" sort="Jacob, A P" uniqKey="Jacob A" first="A. P." last="Jacob">A. P. Jacob</name><name sortKey="Kiss, L L" sort="Kiss, L L" uniqKey="Kiss L" first="L. L." last="Kiss">L. L. Kiss</name><name sortKey="Stello, D" sort="Stello, D" uniqKey="Stello D" first="D." last="Stello">D. Stello</name></country><country name="Danemark"><noRegion><name sortKey="Stello, D" sort="Stello, D" uniqKey="Stello D" first="D." last="Stello">D. Stello</name></noRegion><name sortKey="Arentoft, T" sort="Arentoft, T" uniqKey="Arentoft T" first="T." last="Arentoft">T. Arentoft</name><name sortKey="Arentoft, T" sort="Arentoft, T" uniqKey="Arentoft T" first="T." last="Arentoft">T. Arentoft</name><name sortKey="Frandsen, S" sort="Frandsen, S" uniqKey="Frandsen S" first="S." last="Frandsen">S. Frandsen</name><name sortKey="Frandsen, S" sort="Frandsen, S" uniqKey="Frandsen S" first="S." last="Frandsen">S. Frandsen</name><name sortKey="Jensen, H R" sort="Jensen, H R" uniqKey="Jensen H" first="H. R." last="Jensen">H. R. Jensen</name><name sortKey="Kjeldsen, H" sort="Kjeldsen, H" uniqKey="Kjeldsen H" first="H." last="Kjeldsen">H. Kjeldsen</name><name sortKey="Kjeldsen, H" sort="Kjeldsen, H" uniqKey="Kjeldsen H" first="H." last="Kjeldsen">H. Kjeldsen</name></country><country name="États-Unis"><region name="Colorado"><name sortKey="Stello, D" sort="Stello, D" uniqKey="Stello D" first="D." last="Stello">D. Stello</name></region><name sortKey="Dall, T H" sort="Dall, T H" uniqKey="Dall T" first="T. H." last="Dall">T. H. Dall</name><name sortKey="Gilliland, R L" sort="Gilliland, R L" uniqKey="Gilliland R" first="R. L." last="Gilliland">R. L. Gilliland</name><name sortKey="Szab, R" sort="Szab, R" uniqKey="Szab R" first="R." last="Szab">R. Szab</name></country><country name="Espagne"><noRegion><name sortKey="Suarez, J C" sort="Suarez, J C" uniqKey="Suarez J" first="J. C." last="Suárez">J. C. Suárez</name></noRegion></country><country name="France"><noRegion><name sortKey="Suarez, J C" sort="Suarez, J C" uniqKey="Suarez J" first="J. C." last="Suárez">J. C. Suárez</name></noRegion></country><country name="Belgique"><noRegion><name sortKey="Bouzid, M Y" sort="Bouzid, M Y" uniqKey="Bouzid M" first="M. Y." last="Bouzid">M. Y. Bouzid</name></noRegion><name sortKey="Sterken, C" sort="Sterken, C" uniqKey="Sterken C" first="C." last="Sterken">C. Sterken</name></country><country name="Hongrie"><noRegion><name sortKey="Csubry, Z" sort="Csubry, Z" uniqKey="Csubry Z" first="Z." last="Csubry">Z. Csubry</name></noRegion><name sortKey="Nuspl, J" sort="Nuspl, J" uniqKey="Nuspl J" first="J." last="Nuspl">J. Nuspl</name><name sortKey="Szab, R" sort="Szab, R" uniqKey="Szab R" first="R." last="Szab">R. Szab</name></country><country name="Chili"><noRegion><name sortKey="Dall, T H" sort="Dall, T H" uniqKey="Dall T" first="T. H." last="Dall">T. H. Dall</name></noRegion></country><country name="Corée du Sud"><noRegion><name sortKey="Kang, Y B" sort="Kang, Y B" uniqKey="Kang Y" first="Y. B." last="Kang">Y. B. Kang</name></noRegion><name sortKey="Kim, S" sort="Kim, S" uniqKey="Kim S" first="S." last="Kim">S. Kim</name><name sortKey="Koo, J" sort="Koo, J" uniqKey="Koo J" first="J." last="Koo">J. Koo</name><name sortKey="Lee, C" sort="Lee, C" uniqKey="Lee C" first="C." last="Lee">C. Lee</name><name sortKey="Lee, J" sort="Lee, J" uniqKey="Lee J" first="J." last="Lee">J. Lee</name></country></tree></affiliations></record>Pour manipuler ce document sous Unix (Dilib)
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