MODELING KEPLER OBSERVATIONS OF SOLAR-LIKE OSCILLATIONS IN THE RED GIANT STAR HD 186355
Identifieur interne : 006935 ( Main/Exploration ); précédent : 006934; suivant : 006936MODELING KEPLER OBSERVATIONS OF SOLAR-LIKE OSCILLATIONS IN THE RED GIANT STAR HD 186355
Auteurs : C. Jiang [République populaire de Chine] ; B. W. Jiang [République populaire de Chine] ; J. Christensen-Dalsgaard [Danemark] ; T. R. Bedding [Australie] ; D. Stello [Australie] ; D. Huber [Australie] ; S. Frandsen [Danemark] ; H. Kjeldsen [Danemark] ; C. Karoff [Danemark] ; B. Mosser [France] ; P. Demarque [États-Unis] ; M. N. Fanelli [États-Unis] ; K. Kinemuchi [États-Unis] ; F. Mullally [États-Unis]Source :
- The Astrophysical journal [ 0004-637X ] ; 2011.
Descripteurs français
- Pascal (Inist)
English descriptors
- KwdEn :
Abstract
We have analyzed oscillations of the red giant star HD 186355 observed by the NASA Kepler satellite. The data consist of the first five quarters of science operations of Kepler, which cover about 13 months. The high-precision time-series data allow us to accurately extract the oscillation frequencies from the power spectrum. We find that the frequency of the maximum oscillation power, νmax, and the mean large frequency separation, Δν, are around 106 and 9.4 μHz, respectively. A regular pattern of radial and non-radial oscillation modes is identified by stacking the power spectra in an echelle diagram. We use the scaling relations of Δν and νmax to estimate the preliminary asteroseismic mass, which is confirmed with the modeling result (M = 1.45 ± 0.05 M◦.) using the Yale Rotating stellar Evolution Code (YREC7). In addition, we constrain the effective temperature, luminosity, and radius from comparisons between observational constraints and models. A number of mixed l = 1 modes are also detected and taken into account in our model comparisons. We find a mean observational period spacing for these mixed modes of about 58 s, suggesting that this red giant branch star is in the shell hydrogen-burning phase.
Affiliations:
- Australie, Danemark, France, République populaire de Chine, États-Unis
- Nouvelle-Galles du Sud, Île-de-France
- Paris, Pékin, Sydney
- Université Pierre-et-Marie-Curie, Université de Sydney
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<record><TEI><teiHeader><fileDesc><titleStmt><title xml:lang="en" level="a">MODELING KEPLER OBSERVATIONS OF SOLAR-LIKE OSCILLATIONS IN THE RED GIANT STAR HD 186355</title><author><name sortKey="Jiang, C" sort="Jiang, C" uniqKey="Jiang C" first="C." last="Jiang">C. Jiang</name><affiliation wicri:level="1"><inist:fA14 i1="01"><s1>Department of Astronomy, Beijing Normal University</s1><s2>Beijing 100875</s2><s3>CHN</s3><sZ>1 aut.</sZ><sZ>2 aut.</sZ></inist:fA14><country>République populaire de Chine</country><placeName><settlement type="city">Pékin</settlement></placeName></affiliation></author><author><name sortKey="Jiang, B W" sort="Jiang, B W" uniqKey="Jiang B" first="B. W." last="Jiang">B. W. Jiang</name><affiliation wicri:level="1"><inist:fA14 i1="01"><s1>Department of Astronomy, Beijing Normal University</s1><s2>Beijing 100875</s2><s3>CHN</s3><sZ>1 aut.</sZ><sZ>2 aut.</sZ></inist:fA14><country>République populaire de Chine</country><placeName><settlement type="city">Pékin</settlement></placeName></affiliation></author><author><name sortKey="Christensen Dalsgaard, J" sort="Christensen Dalsgaard, J" uniqKey="Christensen Dalsgaard J" first="J." last="Christensen-Dalsgaard">J. Christensen-Dalsgaard</name><affiliation wicri:level="1"><inist:fA14 i1="02"><s1>Department of Physics and Astronomy, Aarhus University</s1><s2>8000 Aarhus C</s2><s3>DNK</s3><sZ>3 aut.</sZ><sZ>7 aut.</sZ><sZ>8 aut.</sZ><sZ>9 aut.</sZ></inist:fA14><country>Danemark</country><wicri:noRegion>8000 Aarhus C</wicri:noRegion></affiliation></author><author><name sortKey="Bedding, T R" sort="Bedding, T R" uniqKey="Bedding T" first="T. R." last="Bedding">T. R. Bedding</name><affiliation wicri:level="4"><inist:fA14 i1="03"><s1>Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney</s1><s2>Sydney, NSW 2006</s2><s3>AUS</s3><sZ>4 aut.</sZ><sZ>5 aut.</sZ><sZ>6 aut.</sZ></inist:fA14><country>Australie</country><placeName><settlement type="city">Sydney</settlement><region type="état">Nouvelle-Galles du Sud</region></placeName><orgName type="university">Université de Sydney</orgName></affiliation></author><author><name sortKey="Stello, D" sort="Stello, D" uniqKey="Stello D" first="D." last="Stello">D. Stello</name><affiliation wicri:level="4"><inist:fA14 i1="03"><s1>Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney</s1><s2>Sydney, NSW 2006</s2><s3>AUS</s3><sZ>4 aut.</sZ><sZ>5 aut.</sZ><sZ>6 aut.</sZ></inist:fA14><country>Australie</country><placeName><settlement type="city">Sydney</settlement><region type="état">Nouvelle-Galles du Sud</region></placeName><orgName type="university">Université de Sydney</orgName></affiliation></author><author><name sortKey="Huber, D" sort="Huber, D" uniqKey="Huber D" first="D." last="Huber">D. Huber</name><affiliation wicri:level="4"><inist:fA14 i1="03"><s1>Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney</s1><s2>Sydney, NSW 2006</s2><s3>AUS</s3><sZ>4 aut.</sZ><sZ>5 aut.</sZ><sZ>6 aut.</sZ></inist:fA14><country>Australie</country><placeName><settlement type="city">Sydney</settlement><region type="état">Nouvelle-Galles du Sud</region></placeName><orgName type="university">Université de Sydney</orgName></affiliation></author><author><name sortKey="Frandsen, S" sort="Frandsen, S" uniqKey="Frandsen S" first="S." last="Frandsen">S. Frandsen</name><affiliation wicri:level="1"><inist:fA14 i1="02"><s1>Department of Physics and Astronomy, Aarhus University</s1><s2>8000 Aarhus C</s2><s3>DNK</s3><sZ>3 aut.</sZ><sZ>7 aut.</sZ><sZ>8 aut.</sZ><sZ>9 aut.</sZ></inist:fA14><country>Danemark</country><wicri:noRegion>8000 Aarhus C</wicri:noRegion></affiliation></author><author><name sortKey="Kjeldsen, H" sort="Kjeldsen, H" uniqKey="Kjeldsen H" first="H." last="Kjeldsen">H. Kjeldsen</name><affiliation wicri:level="1"><inist:fA14 i1="02"><s1>Department of Physics and Astronomy, Aarhus University</s1><s2>8000 Aarhus C</s2><s3>DNK</s3><sZ>3 aut.</sZ><sZ>7 aut.</sZ><sZ>8 aut.</sZ><sZ>9 aut.</sZ></inist:fA14><country>Danemark</country><wicri:noRegion>8000 Aarhus C</wicri:noRegion></affiliation></author><author><name sortKey="Karoff, C" sort="Karoff, C" uniqKey="Karoff C" first="C." last="Karoff">C. Karoff</name><affiliation wicri:level="1"><inist:fA14 i1="02"><s1>Department of Physics and Astronomy, Aarhus University</s1><s2>8000 Aarhus C</s2><s3>DNK</s3><sZ>3 aut.</sZ><sZ>7 aut.</sZ><sZ>8 aut.</sZ><sZ>9 aut.</sZ></inist:fA14><country>Danemark</country><wicri:noRegion>8000 Aarhus C</wicri:noRegion></affiliation></author><author><name sortKey="Mosser, B" sort="Mosser, B" uniqKey="Mosser B" first="B." last="Mosser">B. Mosser</name><affiliation wicri:level="4"><inist:fA14 i1="04"><s1>LESIA, CNRS, Université Pierre et Marie Curie, Université Denis Diderot, Observatoire de Paris</s1><s2>92195 Meudon</s2><s3>FRA</s3><sZ>10 aut.</sZ></inist:fA14><country>France</country><wicri:noRegion>92195 Meudon</wicri:noRegion><wicri:noRegion>Observatoire de Paris</wicri:noRegion><wicri:noRegion>92195 Meudon</wicri:noRegion><orgName type="university">Université Pierre-et-Marie-Curie</orgName><placeName><settlement type="city">Paris</settlement><region type="region" nuts="2">Île-de-France</region></placeName></affiliation></author><author><name sortKey="Demarque, P" sort="Demarque, P" uniqKey="Demarque P" first="P." last="Demarque">P. Demarque</name><affiliation wicri:level="1"><inist:fA14 i1="05"><s1>Department of Astronomy, Yale University</s1><s2>New Haven, CT 06520-8101</s2><s3>USA</s3><sZ>11 aut.</sZ></inist:fA14><country>États-Unis</country><wicri:noRegion>New Haven, CT 06520-8101</wicri:noRegion></affiliation></author><author><name sortKey="Fanelli, M N" sort="Fanelli, M N" uniqKey="Fanelli M" first="M. N." last="Fanelli">M. N. Fanelli</name><affiliation wicri:level="1"><inist:fA14 i1="06"><s1>Bay Area Environmental Research Institute, NASA Ames Research Center</s1><s2>Moffett Field, CA 94035</s2><s3>USA</s3><sZ>12 aut.</sZ><sZ>13 aut.</sZ></inist:fA14><country>États-Unis</country><wicri:noRegion>Moffett Field, CA 94035</wicri:noRegion></affiliation></author><author><name sortKey="Kinemuchi, K" sort="Kinemuchi, K" uniqKey="Kinemuchi K" first="K." last="Kinemuchi">K. Kinemuchi</name><affiliation wicri:level="1"><inist:fA14 i1="06"><s1>Bay Area Environmental Research Institute, NASA Ames Research Center</s1><s2>Moffett Field, CA 94035</s2><s3>USA</s3><sZ>12 aut.</sZ><sZ>13 aut.</sZ></inist:fA14><country>États-Unis</country><wicri:noRegion>Moffett Field, CA 94035</wicri:noRegion></affiliation></author><author><name sortKey="Mullally, F" sort="Mullally, F" uniqKey="Mullally F" first="F." last="Mullally">F. Mullally</name><affiliation wicri:level="1"><inist:fA14 i1="07"><s1>SETI Institute, NASA Ames Research Center</s1><s2>Moffett Field, CA 94035</s2><s3>USA</s3><sZ>14 aut.</sZ></inist:fA14><country>États-Unis</country><wicri:noRegion>Moffett Field, CA 94035</wicri:noRegion></affiliation></author></titleStmt><publicationStmt><idno type="wicri:source">INIST</idno><idno type="inist">12-0025843</idno><date when="2011">2011</date><idno type="stanalyst">PASCAL 12-0025843 INIST</idno><idno type="RBID">Pascal:12-0025843</idno><idno type="wicri:Area/PascalFrancis/Corpus">001712</idno><idno type="wicri:Area/PascalFrancis/Curation">004797</idno><idno type="wicri:Area/PascalFrancis/Checkpoint">001915</idno><idno type="wicri:explorRef" wicri:stream="PascalFrancis" wicri:step="Checkpoint">001915</idno><idno type="wicri:doubleKey">0004-637X:2011:Jiang C:modeling:kepler:observations</idno><idno type="wicri:Area/Main/Merge">006D66</idno><idno type="wicri:Area/Main/Curation">006935</idno><idno type="wicri:Area/Main/Exploration">006935</idno></publicationStmt><sourceDesc><biblStruct><analytic><title xml:lang="en" level="a">MODELING KEPLER OBSERVATIONS OF SOLAR-LIKE OSCILLATIONS IN THE RED GIANT STAR HD 186355</title><author><name sortKey="Jiang, C" sort="Jiang, C" uniqKey="Jiang C" first="C." last="Jiang">C. Jiang</name><affiliation wicri:level="1"><inist:fA14 i1="01"><s1>Department of Astronomy, Beijing Normal University</s1><s2>Beijing 100875</s2><s3>CHN</s3><sZ>1 aut.</sZ><sZ>2 aut.</sZ></inist:fA14><country>République populaire de Chine</country><placeName><settlement type="city">Pékin</settlement></placeName></affiliation></author><author><name sortKey="Jiang, B W" sort="Jiang, B W" uniqKey="Jiang B" first="B. W." last="Jiang">B. W. Jiang</name><affiliation wicri:level="1"><inist:fA14 i1="01"><s1>Department of Astronomy, Beijing Normal University</s1><s2>Beijing 100875</s2><s3>CHN</s3><sZ>1 aut.</sZ><sZ>2 aut.</sZ></inist:fA14><country>République populaire de Chine</country><placeName><settlement type="city">Pékin</settlement></placeName></affiliation></author><author><name sortKey="Christensen Dalsgaard, J" sort="Christensen Dalsgaard, J" uniqKey="Christensen Dalsgaard J" first="J." last="Christensen-Dalsgaard">J. Christensen-Dalsgaard</name><affiliation wicri:level="1"><inist:fA14 i1="02"><s1>Department of Physics and Astronomy, Aarhus University</s1><s2>8000 Aarhus C</s2><s3>DNK</s3><sZ>3 aut.</sZ><sZ>7 aut.</sZ><sZ>8 aut.</sZ><sZ>9 aut.</sZ></inist:fA14><country>Danemark</country><wicri:noRegion>8000 Aarhus C</wicri:noRegion></affiliation></author><author><name sortKey="Bedding, T R" sort="Bedding, T R" uniqKey="Bedding T" first="T. R." last="Bedding">T. R. Bedding</name><affiliation wicri:level="4"><inist:fA14 i1="03"><s1>Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney</s1><s2>Sydney, NSW 2006</s2><s3>AUS</s3><sZ>4 aut.</sZ><sZ>5 aut.</sZ><sZ>6 aut.</sZ></inist:fA14><country>Australie</country><placeName><settlement type="city">Sydney</settlement><region type="état">Nouvelle-Galles du Sud</region></placeName><orgName type="university">Université de Sydney</orgName></affiliation></author><author><name sortKey="Stello, D" sort="Stello, D" uniqKey="Stello D" first="D." last="Stello">D. Stello</name><affiliation wicri:level="4"><inist:fA14 i1="03"><s1>Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney</s1><s2>Sydney, NSW 2006</s2><s3>AUS</s3><sZ>4 aut.</sZ><sZ>5 aut.</sZ><sZ>6 aut.</sZ></inist:fA14><country>Australie</country><placeName><settlement type="city">Sydney</settlement><region type="état">Nouvelle-Galles du Sud</region></placeName><orgName type="university">Université de Sydney</orgName></affiliation></author><author><name sortKey="Huber, D" sort="Huber, D" uniqKey="Huber D" first="D." last="Huber">D. Huber</name><affiliation wicri:level="4"><inist:fA14 i1="03"><s1>Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney</s1><s2>Sydney, NSW 2006</s2><s3>AUS</s3><sZ>4 aut.</sZ><sZ>5 aut.</sZ><sZ>6 aut.</sZ></inist:fA14><country>Australie</country><placeName><settlement type="city">Sydney</settlement><region type="état">Nouvelle-Galles du Sud</region></placeName><orgName type="university">Université de Sydney</orgName></affiliation></author><author><name sortKey="Frandsen, S" sort="Frandsen, S" uniqKey="Frandsen S" first="S." last="Frandsen">S. Frandsen</name><affiliation wicri:level="1"><inist:fA14 i1="02"><s1>Department of Physics and Astronomy, Aarhus University</s1><s2>8000 Aarhus C</s2><s3>DNK</s3><sZ>3 aut.</sZ><sZ>7 aut.</sZ><sZ>8 aut.</sZ><sZ>9 aut.</sZ></inist:fA14><country>Danemark</country><wicri:noRegion>8000 Aarhus C</wicri:noRegion></affiliation></author><author><name sortKey="Kjeldsen, H" sort="Kjeldsen, H" uniqKey="Kjeldsen H" first="H." last="Kjeldsen">H. Kjeldsen</name><affiliation wicri:level="1"><inist:fA14 i1="02"><s1>Department of Physics and Astronomy, Aarhus University</s1><s2>8000 Aarhus C</s2><s3>DNK</s3><sZ>3 aut.</sZ><sZ>7 aut.</sZ><sZ>8 aut.</sZ><sZ>9 aut.</sZ></inist:fA14><country>Danemark</country><wicri:noRegion>8000 Aarhus C</wicri:noRegion></affiliation></author><author><name sortKey="Karoff, C" sort="Karoff, C" uniqKey="Karoff C" first="C." last="Karoff">C. Karoff</name><affiliation wicri:level="1"><inist:fA14 i1="02"><s1>Department of Physics and Astronomy, Aarhus University</s1><s2>8000 Aarhus C</s2><s3>DNK</s3><sZ>3 aut.</sZ><sZ>7 aut.</sZ><sZ>8 aut.</sZ><sZ>9 aut.</sZ></inist:fA14><country>Danemark</country><wicri:noRegion>8000 Aarhus C</wicri:noRegion></affiliation></author><author><name sortKey="Mosser, B" sort="Mosser, B" uniqKey="Mosser B" first="B." last="Mosser">B. Mosser</name><affiliation wicri:level="4"><inist:fA14 i1="04"><s1>LESIA, CNRS, Université Pierre et Marie Curie, Université Denis Diderot, Observatoire de Paris</s1><s2>92195 Meudon</s2><s3>FRA</s3><sZ>10 aut.</sZ></inist:fA14><country>France</country><wicri:noRegion>92195 Meudon</wicri:noRegion><wicri:noRegion>Observatoire de Paris</wicri:noRegion><wicri:noRegion>92195 Meudon</wicri:noRegion><orgName type="university">Université Pierre-et-Marie-Curie</orgName><placeName><settlement type="city">Paris</settlement><region type="region" nuts="2">Île-de-France</region></placeName></affiliation></author><author><name sortKey="Demarque, P" sort="Demarque, P" uniqKey="Demarque P" first="P." last="Demarque">P. Demarque</name><affiliation wicri:level="1"><inist:fA14 i1="05"><s1>Department of Astronomy, Yale University</s1><s2>New Haven, CT 06520-8101</s2><s3>USA</s3><sZ>11 aut.</sZ></inist:fA14><country>États-Unis</country><wicri:noRegion>New Haven, CT 06520-8101</wicri:noRegion></affiliation></author><author><name sortKey="Fanelli, M N" sort="Fanelli, M N" uniqKey="Fanelli M" first="M. N." last="Fanelli">M. N. Fanelli</name><affiliation wicri:level="1"><inist:fA14 i1="06"><s1>Bay Area Environmental Research Institute, NASA Ames Research Center</s1><s2>Moffett Field, CA 94035</s2><s3>USA</s3><sZ>12 aut.</sZ><sZ>13 aut.</sZ></inist:fA14><country>États-Unis</country><wicri:noRegion>Moffett Field, CA 94035</wicri:noRegion></affiliation></author><author><name sortKey="Kinemuchi, K" sort="Kinemuchi, K" uniqKey="Kinemuchi K" first="K." last="Kinemuchi">K. Kinemuchi</name><affiliation wicri:level="1"><inist:fA14 i1="06"><s1>Bay Area Environmental Research Institute, NASA Ames Research Center</s1><s2>Moffett Field, CA 94035</s2><s3>USA</s3><sZ>12 aut.</sZ><sZ>13 aut.</sZ></inist:fA14><country>États-Unis</country><wicri:noRegion>Moffett Field, CA 94035</wicri:noRegion></affiliation></author><author><name sortKey="Mullally, F" sort="Mullally, F" uniqKey="Mullally F" first="F." last="Mullally">F. Mullally</name><affiliation wicri:level="1"><inist:fA14 i1="07"><s1>SETI Institute, NASA Ames Research Center</s1><s2>Moffett Field, CA 94035</s2><s3>USA</s3><sZ>14 aut.</sZ></inist:fA14><country>États-Unis</country><wicri:noRegion>Moffett Field, CA 94035</wicri:noRegion></affiliation></author></analytic><series><title level="j" type="main">The Astrophysical journal</title><title level="j" type="abbreviated">Astrophys. j.</title><idno type="ISSN">0004-637X</idno><imprint><date when="2011">2011</date></imprint></series></biblStruct></sourceDesc><seriesStmt><title level="j" type="main">The Astrophysical journal</title><title level="j" type="abbreviated">Astrophys. j.</title><idno type="ISSN">0004-637X</idno></seriesStmt></fileDesc><profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>Data analysis</term><term>Effective temperature</term><term>Giant stars</term><term>Hydrogen burning</term><term>Kepler satellite</term><term>Luminosity</term><term>Modelling</term><term>Models</term><term>Oscillation frequency</term><term>Oscillation modes</term><term>Power spectra</term><term>Red giant stars</term><term>Red stars</term><term>Solar type star</term><term>Stellar evolution</term><term>Time series</term></keywords><keywords scheme="Pascal" xml:lang="fr"><term>Modélisation</term><term>Etoile rouge</term><term>Géante rouge</term><term>Etoile géante</term><term>Satellite Kepler</term><term>Série temporelle</term><term>Fréquence oscillation</term><term>Spectre puissance</term><term>Mode oscillation</term><term>Evolution stellaire</term><term>Température effective</term><term>Luminosité</term><term>Modèle</term><term>Combustion hydrogène</term><term>Analyse donnée</term><term>Etoile type solaire</term></keywords></textClass></profileDesc></teiHeader><front><div type="abstract" xml:lang="en">We have analyzed oscillations of the red giant star HD 186355 observed by the NASA Kepler satellite. The data consist of the first five quarters of science operations of Kepler, which cover about 13 months. The high-precision time-series data allow us to accurately extract the oscillation frequencies from the power spectrum. We find that the frequency of the maximum oscillation power, ν<sub>max</sub>, and the mean large frequency separation, Δν, are around 106 and 9.4 μHz, respectively. A regular pattern of radial and non-radial oscillation modes is identified by stacking the power spectra in an echelle diagram. We use the scaling relations of Δν and ν<sub>max</sub> to estimate the preliminary asteroseismic mass, which is confirmed with the modeling result (M = 1.45 ± 0.05 M<sub>◦.</sub>) using the Yale Rotating stellar Evolution Code (YREC7). In addition, we constrain the effective temperature, luminosity, and radius from comparisons between observational constraints and models. A number of mixed l = 1 modes are also detected and taken into account in our model comparisons. We find a mean observational period spacing for these mixed modes of about 58 s, suggesting that this red giant branch star is in the shell hydrogen-burning phase.</div></front></TEI><affiliations><list><country><li>Australie</li><li>Danemark</li><li>France</li><li>République populaire de Chine</li><li>États-Unis</li></country><region><li>Nouvelle-Galles du Sud</li><li>Île-de-France</li></region><settlement><li>Paris</li><li>Pékin</li><li>Sydney</li></settlement><orgName><li>Université Pierre-et-Marie-Curie</li><li>Université de Sydney</li></orgName></list><tree><country name="République populaire de Chine"><noRegion><name sortKey="Jiang, C" sort="Jiang, C" uniqKey="Jiang C" first="C." last="Jiang">C. Jiang</name></noRegion><name sortKey="Jiang, B W" sort="Jiang, B W" uniqKey="Jiang B" first="B. W." last="Jiang">B. W. Jiang</name></country><country name="Danemark"><noRegion><name sortKey="Christensen Dalsgaard, J" sort="Christensen Dalsgaard, J" uniqKey="Christensen Dalsgaard J" first="J." last="Christensen-Dalsgaard">J. Christensen-Dalsgaard</name></noRegion><name sortKey="Frandsen, S" sort="Frandsen, S" uniqKey="Frandsen S" first="S." last="Frandsen">S. Frandsen</name><name sortKey="Karoff, C" sort="Karoff, C" uniqKey="Karoff C" first="C." last="Karoff">C. Karoff</name><name sortKey="Kjeldsen, H" sort="Kjeldsen, H" uniqKey="Kjeldsen H" first="H." last="Kjeldsen">H. Kjeldsen</name></country><country name="Australie"><region name="Nouvelle-Galles du Sud"><name sortKey="Bedding, T R" sort="Bedding, T R" uniqKey="Bedding T" first="T. R." last="Bedding">T. R. Bedding</name></region><name sortKey="Huber, D" sort="Huber, D" uniqKey="Huber D" first="D." last="Huber">D. Huber</name><name sortKey="Stello, D" sort="Stello, D" uniqKey="Stello D" first="D." last="Stello">D. Stello</name></country><country name="France"><region name="Île-de-France"><name sortKey="Mosser, B" sort="Mosser, B" uniqKey="Mosser B" first="B." last="Mosser">B. Mosser</name></region></country><country name="États-Unis"><noRegion><name sortKey="Demarque, P" sort="Demarque, P" uniqKey="Demarque P" first="P." last="Demarque">P. Demarque</name></noRegion><name sortKey="Fanelli, M N" sort="Fanelli, M N" uniqKey="Fanelli M" first="M. N." last="Fanelli">M. N. Fanelli</name><name sortKey="Kinemuchi, K" sort="Kinemuchi, K" uniqKey="Kinemuchi K" first="K." last="Kinemuchi">K. Kinemuchi</name><name sortKey="Mullally, F" sort="Mullally, F" uniqKey="Mullally F" first="F." last="Mullally">F. Mullally</name></country></tree></affiliations></record>Pour manipuler ce document sous Unix (Dilib)
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