CONSTRUCTING A ONE-SOLAR-MASS EVOLUTIONARY SEQUENCE USING ASTEROSEISMIC DATA FROM KEPLER
Identifieur interne : 004674 ( PascalFrancis/Curation ); précédent : 004673; suivant : 004675CONSTRUCTING A ONE-SOLAR-MASS EVOLUTIONARY SEQUENCE USING ASTEROSEISMIC DATA FROM KEPLER
Auteurs : V. Silva Aguirre [Allemagne] ; W. J. Chaplin [Royaume-Uni] ; J. Ballot [France] ; S. Basu [États-Unis] ; T. R. Bedding [Australie] ; A. M. Serenelli [Espagne] ; G. A. Verner [Royaume-Uni] ; A. Miglio [Royaume-Uni] ; M. J. P. F. G. Monteiro [Portugal] ; A. Weiss [Allemagne] ; T. Appourchaux [France] ; A. Bonanno [Italie] ; A. M. Broomhall [Royaume-Uni] ; H. Bruntt [Danemark] ; T. L. Campante [Portugal, Danemark] ; L. Casagrande [Allemagne] ; E. Corsaro [Italie] ; Y. Elsworth [Royaume-Uni] ; R. A. Garcia [France] ; P. Gaulme [France] ; R. Handberg [Danemark] ; S. Hekker [Royaume-Uni, Pays-Bas] ; D. Huber [Australie] ; C. Karoff [Danemark] ; S. Mathur [États-Unis] ; B. Mosser [France] ; D. Salabert [France] ; R. Schönrich [Allemagne] ; S. G. Sousa [Portugal] ; D. Stello [Australie] ; T. R. White [Australie] ; J. Christensen-Dalsgaard [Danemark] ; R. L. Gilliland [États-Unis] ; S. D. Kawaler [États-Unis] ; H. Kjeldsen [Danemark] ; G. Houdek [Autriche] ; T. S. Metcalfe [États-Unis] ; J. Molenda-Zakowicz [Pologne] ; M. J. Thompson [États-Unis] ; D. A. Caldwell [États-Unis] ; J. L. Christiansen [États-Unis] ; B. Wohler [États-Unis]Source :
- The Astrophysical journal [ 0004-637X ] ; 2011.
Descripteurs français
- Pascal (Inist)
English descriptors
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Abstract
Asteroseismology of solar-type stars has entered a new era of large surveys with the success of the NASA Kepler mission, which is providing exquisite data on oscillations of stars across the Hertzsprung-Russell diagram. From the time-series photometry, the two seismic parameters that can be most readily extracted are the large frequency separation (Δν) and the frequency of maximum oscillation power (νmax). After the survey phase, these quantities are available for hundreds of solar-type stars. By scaling from solar values, we use these two asteroseismic observables to identify for the first time an evolutionary sequence of 1 M◦. field stars, without the need for further information from stellar models. Comparison of our determinations with the few available spectroscopic results shows an excellent level of agreement. We discuss the potential of the method for differential analysis throughout the main-sequence evolution and the possibility of detecting twins of very well-known stars.
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<sZ>34 aut.</sZ>
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<affiliation wicri:level="1"><inist:fA14 i1="12"><s1>Department of Physics and Astronomy, Aarhus University</s1>
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</author>
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<affiliation wicri:level="1"><inist:fA14 i1="15"><s1>High Altitude Observatory, NCAR, P.O. Box 3000</s1>
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<affiliation wicri:level="1"><inist:fA14 i1="22"><s1>Instytut Astronomiczny Uniwersytetu Wroclawskiego, ul. Kopemika 11</s1>
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<sZ>38 aut.</sZ>
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<country>Pologne</country>
</affiliation>
</author>
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<affiliation wicri:level="1"><inist:fA14 i1="15"><s1>High Altitude Observatory, NCAR, P.O. Box 3000</s1>
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<sZ>25 aut.</sZ>
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<author><name sortKey="Caldwell, D A" sort="Caldwell, D A" uniqKey="Caldwell D" first="D. A." last="Caldwell">D. A. Caldwell</name>
<affiliation wicri:level="1"><inist:fA14 i1="23"><s1>SETI Institute/NASA Ames Research Center</s1>
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<sZ>40 aut.</sZ>
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<author><name sortKey="Christiansen, J L" sort="Christiansen, J L" uniqKey="Christiansen J" first="J. L." last="Christiansen">J. L. Christiansen</name>
<affiliation wicri:level="1"><inist:fA14 i1="23"><s1>SETI Institute/NASA Ames Research Center</s1>
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<sZ>40 aut.</sZ>
<sZ>41 aut.</sZ>
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</author>
<author><name sortKey="Wohler, B" sort="Wohler, B" uniqKey="Wohler B" first="B." last="Wohler">B. Wohler</name>
<affiliation wicri:level="1"><inist:fA14 i1="24"><s1>Orbital Sciences Corporation/NASA Ames Research Center</s1>
<s2>Moffett Field, CA 94035</s2>
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<sZ>42 aut.</sZ>
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<country>États-Unis</country>
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</titleStmt>
<publicationStmt><idno type="wicri:source">INIST</idno>
<idno type="inist">11-0466018</idno>
<date when="2011">2011</date>
<idno type="stanalyst">PASCAL 11-0466018 INIST</idno>
<idno type="RBID">Pascal:11-0466018</idno>
<idno type="wicri:Area/PascalFrancis/Corpus">001882</idno>
<idno type="wicri:Area/PascalFrancis/Curation">004674</idno>
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<sourceDesc><biblStruct><analytic><title xml:lang="en" level="a">CONSTRUCTING A ONE-SOLAR-MASS EVOLUTIONARY SEQUENCE USING ASTEROSEISMIC DATA FROM KEPLER</title>
<author><name sortKey="Aguirre, V Silva" sort="Aguirre, V Silva" uniqKey="Aguirre V" first="V. Silva" last="Aguirre">V. Silva Aguirre</name>
<affiliation wicri:level="1"><inist:fA14 i1="01"><s1>Max Planck Institute for Astrophysics, Karl-Schwarzschild-Str 1, 85748</s1>
<s2>Garching bei München</s2>
<s3>DEU</s3>
<sZ>1 aut.</sZ>
<sZ>10 aut.</sZ>
<sZ>16 aut.</sZ>
<sZ>28 aut.</sZ>
</inist:fA14>
<country>Allemagne</country>
</affiliation>
</author>
<author><name sortKey="Chaplin, W J" sort="Chaplin, W J" uniqKey="Chaplin W" first="W. J." last="Chaplin">W. J. Chaplin</name>
<affiliation wicri:level="1"><inist:fA14 i1="02"><s1>School of Physics and Astronomy, University of Birmingham</s1>
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<sZ>2 aut.</sZ>
<sZ>7 aut.</sZ>
<sZ>8 aut.</sZ>
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<country>Royaume-Uni</country>
</affiliation>
</author>
<author><name sortKey="Ballot, J" sort="Ballot, J" uniqKey="Ballot J" first="J." last="Ballot">J. Ballot</name>
<affiliation wicri:level="1"><inist:fA14 i1="03"><s1>Institut de Recherche en Astrophysique et Planetologie, CNRS, 14 avenue Edouard Belin</s1>
<s2>31400 Toulouse</s2>
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<sZ>3 aut.</sZ>
</inist:fA14>
<country>France</country>
</affiliation>
<affiliation wicri:level="1"><inist:fA14 i1="04"><s1>Universite de Toulouse, UPS-OMP, Institut de Recherche en Astrophysique et Planétologie</s1>
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<sZ>3 aut.</sZ>
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<country>France</country>
</affiliation>
</author>
<author><name sortKey="Basu, S" sort="Basu, S" uniqKey="Basu S" first="S." last="Basu">S. Basu</name>
<affiliation wicri:level="1"><inist:fA14 i1="05"><s1>Department of Astronomy, Yale University, P.O. Box 208101</s1>
<s2>New Haven, CT 06520-8101</s2>
<s3>USA</s3>
<sZ>4 aut.</sZ>
</inist:fA14>
<country>États-Unis</country>
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</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="1"><inist:fA14 i1="06"><s1>Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney</s1>
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</author>
<author><name sortKey="Serenelli, A M" sort="Serenelli, A M" uniqKey="Serenelli A" first="A. M." last="Serenelli">A. M. Serenelli</name>
<affiliation wicri:level="1"><inist:fA14 i1="07"><s1>Instituto de Ciencias del Espacio (CSIC-IEEC), Facultad de Ciències, Campus UAB</s1>
<s2>08193 Bellaterra</s2>
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<sZ>6 aut.</sZ>
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<country>Espagne</country>
</affiliation>
</author>
<author><name sortKey="Verner, G A" sort="Verner, G A" uniqKey="Verner G" first="G. A." last="Verner">G. A. Verner</name>
<affiliation wicri:level="1"><inist:fA14 i1="02"><s1>School of Physics and Astronomy, University of Birmingham</s1>
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<sZ>2 aut.</sZ>
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<country>Royaume-Uni</country>
</affiliation>
<affiliation wicri:level="1"><inist:fA14 i1="08"><s1>Astronomy Unit, Queen Mary University of London</s1>
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<sZ>7 aut.</sZ>
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<country>Royaume-Uni</country>
</affiliation>
</author>
<author><name sortKey="Miglio, A" sort="Miglio, A" uniqKey="Miglio A" first="A." last="Miglio">A. Miglio</name>
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<sZ>2 aut.</sZ>
<sZ>7 aut.</sZ>
<sZ>8 aut.</sZ>
<sZ>13 aut.</sZ>
<sZ>18 aut.</sZ>
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<country>Royaume-Uni</country>
</affiliation>
</author>
<author><name sortKey="Monteiro, M J P F G" sort="Monteiro, M J P F G" uniqKey="Monteiro M" first="M. J. P. F. G." last="Monteiro">M. J. P. F. G. Monteiro</name>
<affiliation wicri:level="1"><inist:fA14 i1="09"><s1>Centre de Astrofísica and Faculdade de Ciencias, Universidade do Porto, Rua das Estrelas</s1>
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<sZ>9 aut.</sZ>
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<country>Portugal</country>
</affiliation>
</author>
<author><name sortKey="Weiss, A" sort="Weiss, A" uniqKey="Weiss A" first="A." last="Weiss">A. Weiss</name>
<affiliation wicri:level="1"><inist:fA14 i1="01"><s1>Max Planck Institute for Astrophysics, Karl-Schwarzschild-Str 1, 85748</s1>
<s2>Garching bei München</s2>
<s3>DEU</s3>
<sZ>1 aut.</sZ>
<sZ>10 aut.</sZ>
<sZ>16 aut.</sZ>
<sZ>28 aut.</sZ>
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<country>Allemagne</country>
</affiliation>
</author>
<author><name sortKey="Appourchaux, T" sort="Appourchaux, T" uniqKey="Appourchaux T" first="T." last="Appourchaux">T. Appourchaux</name>
<affiliation wicri:level="1"><inist:fA14 i1="10"><s1>Institut d'Astrophysique Spatiale Universit Paris 11-CNRS (UMR8617) Batiment 121</s1>
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<sZ>11 aut.</sZ>
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<country>France</country>
</affiliation>
</author>
<author><name sortKey="Bonanno, A" sort="Bonanno, A" uniqKey="Bonanno A" first="A." last="Bonanno">A. Bonanno</name>
<affiliation wicri:level="1"><inist:fA14 i1="11"><s1>INAF-Osservatorio Astrofisico di Catania, Via S. Sofia 78</s1>
<s2>95123 Catania</s2>
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<sZ>12 aut.</sZ>
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<country>Italie</country>
</affiliation>
</author>
<author><name sortKey="Broomhall, A M" sort="Broomhall, A M" uniqKey="Broomhall A" first="A. M." last="Broomhall">A. M. Broomhall</name>
<affiliation wicri:level="1"><inist:fA14 i1="02"><s1>School of Physics and Astronomy, University of Birmingham</s1>
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<sZ>2 aut.</sZ>
<sZ>7 aut.</sZ>
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<country>Royaume-Uni</country>
</affiliation>
</author>
<author><name sortKey="Bruntt, H" sort="Bruntt, H" uniqKey="Bruntt H" first="H." last="Bruntt">H. Bruntt</name>
<affiliation wicri:level="1"><inist:fA14 i1="12"><s1>Department of Physics and Astronomy, Aarhus University</s1>
<s2>8000 Aarhus C</s2>
<s3>DNK</s3>
<sZ>14 aut.</sZ>
<sZ>15 aut.</sZ>
<sZ>21 aut.</sZ>
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<country>Danemark</country>
</affiliation>
</author>
<author><name sortKey="Campante, T L" sort="Campante, T L" uniqKey="Campante T" first="T. L." last="Campante">T. L. Campante</name>
<affiliation wicri:level="1"><inist:fA14 i1="09"><s1>Centre de Astrofísica and Faculdade de Ciencias, Universidade do Porto, Rua das Estrelas</s1>
<s2>4150-762 Porto</s2>
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<sZ>9 aut.</sZ>
<sZ>15 aut.</sZ>
<sZ>29 aut.</sZ>
</inist:fA14>
<country>Portugal</country>
</affiliation>
<affiliation wicri:level="1"><inist:fA14 i1="12"><s1>Department of Physics and Astronomy, Aarhus University</s1>
<s2>8000 Aarhus C</s2>
<s3>DNK</s3>
<sZ>14 aut.</sZ>
<sZ>15 aut.</sZ>
<sZ>21 aut.</sZ>
<sZ>24 aut.</sZ>
<sZ>32 aut.</sZ>
<sZ>35 aut.</sZ>
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<country>Danemark</country>
</affiliation>
</author>
<author><name sortKey="Casagrande, L" sort="Casagrande, L" uniqKey="Casagrande L" first="L." last="Casagrande">L. Casagrande</name>
<affiliation wicri:level="1"><inist:fA14 i1="01"><s1>Max Planck Institute for Astrophysics, Karl-Schwarzschild-Str 1, 85748</s1>
<s2>Garching bei München</s2>
<s3>DEU</s3>
<sZ>1 aut.</sZ>
<sZ>10 aut.</sZ>
<sZ>16 aut.</sZ>
<sZ>28 aut.</sZ>
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<country>Allemagne</country>
</affiliation>
</author>
<author><name sortKey="Corsaro, E" sort="Corsaro, E" uniqKey="Corsaro E" first="E." last="Corsaro">E. Corsaro</name>
<affiliation wicri:level="1"><inist:fA14 i1="11"><s1>INAF-Osservatorio Astrofisico di Catania, Via S. Sofia 78</s1>
<s2>95123 Catania</s2>
<s3>ITA</s3>
<sZ>12 aut.</sZ>
<sZ>17 aut.</sZ>
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<country>Italie</country>
</affiliation>
</author>
<author><name sortKey="Elsworth, Y" sort="Elsworth, Y" uniqKey="Elsworth Y" first="Y." last="Elsworth">Y. Elsworth</name>
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<sZ>2 aut.</sZ>
<sZ>7 aut.</sZ>
<sZ>8 aut.</sZ>
<sZ>13 aut.</sZ>
<sZ>18 aut.</sZ>
<sZ>22 aut.</sZ>
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<country>Royaume-Uni</country>
</affiliation>
</author>
<author><name sortKey="Garcia, R A" sort="Garcia, R A" uniqKey="Garcia R" first="R. A." last="Garcia">R. A. Garcia</name>
<affiliation wicri:level="1"><inist:fA14 i1="13"><s1>Laboratoire AIM, CEA/DSM-CNRS-Universite Paris Diderot; IRFU/SAp, Centre de Saclay</s1>
<s2>91191 Gif-sur-Yvette</s2>
<s3>FRA</s3>
<sZ>19 aut.</sZ>
</inist:fA14>
<country>France</country>
</affiliation>
</author>
<author><name sortKey="Gaulme, P" sort="Gaulme, P" uniqKey="Gaulme P" first="P." last="Gaulme">P. Gaulme</name>
<affiliation wicri:level="1"><inist:fA14 i1="10"><s1>Institut d'Astrophysique Spatiale Universit Paris 11-CNRS (UMR8617) Batiment 121</s1>
<s2>91405 ORSAY</s2>
<s3>FRA</s3>
<sZ>11 aut.</sZ>
<sZ>20 aut.</sZ>
</inist:fA14>
<country>France</country>
</affiliation>
</author>
<author><name sortKey="Handberg, R" sort="Handberg, R" uniqKey="Handberg R" first="R." last="Handberg">R. Handberg</name>
<affiliation wicri:level="1"><inist:fA14 i1="12"><s1>Department of Physics and Astronomy, Aarhus University</s1>
<s2>8000 Aarhus C</s2>
<s3>DNK</s3>
<sZ>14 aut.</sZ>
<sZ>15 aut.</sZ>
<sZ>21 aut.</sZ>
<sZ>24 aut.</sZ>
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<sZ>35 aut.</sZ>
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<country>Danemark</country>
</affiliation>
</author>
<author><name sortKey="Hekker, S" sort="Hekker, S" uniqKey="Hekker S" first="S." last="Hekker">S. Hekker</name>
<affiliation wicri:level="1"><inist:fA14 i1="02"><s1>School of Physics and Astronomy, University of Birmingham</s1>
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<sZ>2 aut.</sZ>
<sZ>7 aut.</sZ>
<sZ>8 aut.</sZ>
<sZ>13 aut.</sZ>
<sZ>18 aut.</sZ>
<sZ>22 aut.</sZ>
</inist:fA14>
<country>Royaume-Uni</country>
</affiliation>
<affiliation wicri:level="1"><inist:fA14 i1="14"><s1>Astronomical Institute "Anton Pannekoek," University of Amsterdam, Science Park 904</s1>
<s2>1098 XH Amsterdam</s2>
<s3>NLD</s3>
<sZ>22 aut.</sZ>
</inist:fA14>
<country>Pays-Bas</country>
</affiliation>
</author>
<author><name sortKey="Huber, D" sort="Huber, D" uniqKey="Huber D" first="D." last="Huber">D. Huber</name>
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<sZ>5 aut.</sZ>
<sZ>23 aut.</sZ>
<sZ>30 aut.</sZ>
<sZ>31 aut.</sZ>
</inist:fA14>
<country>Australie</country>
</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="12"><s1>Department of Physics and Astronomy, Aarhus University</s1>
<s2>8000 Aarhus C</s2>
<s3>DNK</s3>
<sZ>14 aut.</sZ>
<sZ>15 aut.</sZ>
<sZ>21 aut.</sZ>
<sZ>24 aut.</sZ>
<sZ>32 aut.</sZ>
<sZ>35 aut.</sZ>
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<country>Danemark</country>
</affiliation>
</author>
<author><name sortKey="Mathur, S" sort="Mathur, S" uniqKey="Mathur S" first="S." last="Mathur">S. Mathur</name>
<affiliation wicri:level="1"><inist:fA14 i1="15"><s1>High Altitude Observatory, NCAR, P.O. Box 3000</s1>
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<sZ>25 aut.</sZ>
<sZ>37 aut.</sZ>
<sZ>39 aut.</sZ>
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<country>États-Unis</country>
</affiliation>
</author>
<author><name sortKey="Mosser, B" sort="Mosser, B" uniqKey="Mosser B" first="B." last="Mosser">B. Mosser</name>
<affiliation wicri:level="1"><inist:fA14 i1="16"><s1>LESIA, CNRS, Universite Pierre et Marie Curie, Universite Denis Diderot, Observatoire de Paris</s1>
<s2>92195 Meudon</s2>
<s3>FRA</s3>
<sZ>26 aut.</sZ>
</inist:fA14>
<country>France</country>
</affiliation>
</author>
<author><name sortKey="Salabert, D" sort="Salabert, D" uniqKey="Salabert D" first="D." last="Salabert">D. Salabert</name>
<affiliation wicri:level="1"><inist:fA14 i1="17"><s1>Universite de Nice Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, BP 4229</s1>
<s2>06304 Nice</s2>
<s3>FRA</s3>
<sZ>27 aut.</sZ>
</inist:fA14>
<country>France</country>
</affiliation>
</author>
<author><name sortKey="Schonrich, R" sort="Schonrich, R" uniqKey="Schonrich R" first="R." last="Schönrich">R. Schönrich</name>
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<sZ>9 aut.</sZ>
<sZ>15 aut.</sZ>
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<author><name sortKey="Stello, D" sort="Stello, D" uniqKey="Stello D" first="D." last="Stello">D. Stello</name>
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<sZ>23 aut.</sZ>
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<author><name sortKey="White, T R" sort="White, T R" uniqKey="White T" first="T. R." last="White">T. R. White</name>
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<sZ>5 aut.</sZ>
<sZ>23 aut.</sZ>
<sZ>30 aut.</sZ>
<sZ>31 aut.</sZ>
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<sZ>31 aut.</sZ>
</inist:fA14>
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<author><name sortKey="Christensen Dalsgaard, J" sort="Christensen Dalsgaard, J" uniqKey="Christensen Dalsgaard J" first="J." last="Christensen-Dalsgaard">J. Christensen-Dalsgaard</name>
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<sZ>34 aut.</sZ>
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<affiliation wicri:level="1"><inist:fA14 i1="15"><s1>High Altitude Observatory, NCAR, P.O. Box 3000</s1>
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<author><name sortKey="Christiansen, J L" sort="Christiansen, J L" uniqKey="Christiansen J" first="J. L." last="Christiansen">J. L. Christiansen</name>
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<affiliation wicri:level="1"><inist:fA14 i1="24"><s1>Orbital Sciences Corporation/NASA Ames Research Center</s1>
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<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>Astroseismology</term>
<term>M stars</term>
<term>Photometry</term>
<term>Solar type star</term>
<term>Star models</term>
<term>Stellar evolution</term>
<term>Time series</term>
</keywords>
<keywords scheme="Pascal" xml:lang="fr"><term>Astéroséismologie</term>
<term>Etoile type solaire</term>
<term>Série temporelle</term>
<term>Photométrie</term>
<term>Etoile M</term>
<term>Modèle stellaire</term>
<term>Evolution stellaire</term>
</keywords>
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<front><div type="abstract" xml:lang="en">Asteroseismology of solar-type stars has entered a new era of large surveys with the success of the NASA Kepler mission, which is providing exquisite data on oscillations of stars across the Hertzsprung-Russell diagram. From the time-series photometry, the two seismic parameters that can be most readily extracted are the large frequency separation (Δν) and the frequency of maximum oscillation power (ν<sub>max</sub>
). After the survey phase, these quantities are available for hundreds of solar-type stars. By scaling from solar values, we use these two asteroseismic observables to identify for the first time an evolutionary sequence of 1 M<sub>◦.</sub>
field stars, without the need for further information from stellar models. Comparison of our determinations with the few available spectroscopic results shows an excellent level of agreement. We discuss the potential of the method for differential analysis throughout the main-sequence evolution and the possibility of detecting twins of very well-known stars.</div>
</front>
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<fA08 i1="01" i2="1" l="ENG"><s1>CONSTRUCTING A ONE-SOLAR-MASS EVOLUTIONARY SEQUENCE USING ASTEROSEISMIC DATA FROM KEPLER</s1>
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<fA11 i1="01" i2="1"><s1>AGUIRRE (V. Silva)</s1>
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<fA14 i1="01"><s1>Max Planck Institute for Astrophysics, Karl-Schwarzschild-Str 1, 85748</s1>
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<sZ>10 aut.</sZ>
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<sZ>7 aut.</sZ>
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<sZ>3 aut.</sZ>
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<fA14 i1="05"><s1>Department of Astronomy, Yale University, P.O. Box 208101</s1>
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<sZ>4 aut.</sZ>
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<fA14 i1="06"><s1>Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney</s1>
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<sZ>23 aut.</sZ>
<sZ>30 aut.</sZ>
<sZ>31 aut.</sZ>
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<sZ>9 aut.</sZ>
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<sZ>12 aut.</sZ>
<sZ>17 aut.</sZ>
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<fA14 i1="12"><s1>Department of Physics and Astronomy, Aarhus University</s1>
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<sZ>14 aut.</sZ>
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<sZ>19 aut.</sZ>
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<fA14 i1="14"><s1>Astronomical Institute "Anton Pannekoek," University of Amsterdam, Science Park 904</s1>
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<s3>NLD</s3>
<sZ>22 aut.</sZ>
</fA14>
<fA14 i1="15"><s1>High Altitude Observatory, NCAR, P.O. Box 3000</s1>
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<sZ>25 aut.</sZ>
<sZ>37 aut.</sZ>
<sZ>39 aut.</sZ>
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<fA14 i1="16"><s1>LESIA, CNRS, Universite Pierre et Marie Curie, Universite Denis Diderot, Observatoire de Paris</s1>
<s2>92195 Meudon</s2>
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<sZ>26 aut.</sZ>
</fA14>
<fA14 i1="17"><s1>Universite de Nice Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, BP 4229</s1>
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<s3>FRA</s3>
<sZ>27 aut.</sZ>
</fA14>
<fA14 i1="18"><s1>Australian Astronomical Observatory, P.O. Box 296</s1>
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<s3>AUS</s3>
<sZ>31 aut.</sZ>
</fA14>
<fA14 i1="19"><s1>Space Telescope Science Institute, 3700 San Martin Drive</s1>
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<sZ>33 aut.</sZ>
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<s2>Ames, IA 50014</s2>
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<sZ>34 aut.</sZ>
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<fA14 i1="21"><s1>Institute of Astronomy, University of Vienna</s1>
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<sZ>36 aut.</sZ>
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<fA14 i1="22"><s1>Instytut Astronomiczny Uniwersytetu Wroclawskiego, ul. Kopemika 11</s1>
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<sZ>38 aut.</sZ>
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<fA14 i1="23"><s1>SETI Institute/NASA Ames Research Center</s1>
<s2>Moffett Field, CA 94035</s2>
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<sZ>40 aut.</sZ>
<sZ>41 aut.</sZ>
</fA14>
<fA14 i1="24"><s1>Orbital Sciences Corporation/NASA Ames Research Center</s1>
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<sZ>42 aut.</sZ>
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<fA66 i1="01"><s0>GBR</s0>
</fA66>
<fC01 i1="01" l="ENG"><s0>Asteroseismology of solar-type stars has entered a new era of large surveys with the success of the NASA Kepler mission, which is providing exquisite data on oscillations of stars across the Hertzsprung-Russell diagram. From the time-series photometry, the two seismic parameters that can be most readily extracted are the large frequency separation (Δν) and the frequency of maximum oscillation power (ν<sub>max</sub>
). After the survey phase, these quantities are available for hundreds of solar-type stars. By scaling from solar values, we use these two asteroseismic observables to identify for the first time an evolutionary sequence of 1 M<sub>◦.</sub>
field stars, without the need for further information from stellar models. Comparison of our determinations with the few available spectroscopic results shows an excellent level of agreement. We discuss the potential of the method for differential analysis throughout the main-sequence evolution and the possibility of detecting twins of very well-known stars.</s0>
</fC01>
<fC02 i1="01" i2="3"><s0>001E03</s0>
</fC02>
<fC03 i1="01" i2="3" l="FRE"><s0>Astéroséismologie</s0>
<s5>26</s5>
</fC03>
<fC03 i1="01" i2="3" l="ENG"><s0>Astroseismology</s0>
<s5>26</s5>
</fC03>
<fC03 i1="02" i2="X" l="FRE"><s0>Etoile type solaire</s0>
<s5>27</s5>
</fC03>
<fC03 i1="02" i2="X" l="ENG"><s0>Solar type star</s0>
<s5>27</s5>
</fC03>
<fC03 i1="02" i2="X" l="SPA"><s0>Estrella tipo solar</s0>
<s5>27</s5>
</fC03>
<fC03 i1="03" i2="3" l="FRE"><s0>Série temporelle</s0>
<s5>28</s5>
</fC03>
<fC03 i1="03" i2="3" l="ENG"><s0>Time series</s0>
<s5>28</s5>
</fC03>
<fC03 i1="04" i2="3" l="FRE"><s0>Photométrie</s0>
<s5>29</s5>
</fC03>
<fC03 i1="04" i2="3" l="ENG"><s0>Photometry</s0>
<s5>29</s5>
</fC03>
<fC03 i1="05" i2="3" l="FRE"><s0>Etoile M</s0>
<s5>30</s5>
</fC03>
<fC03 i1="05" i2="3" l="ENG"><s0>M stars</s0>
<s5>30</s5>
</fC03>
<fC03 i1="06" i2="3" l="FRE"><s0>Modèle stellaire</s0>
<s5>31</s5>
</fC03>
<fC03 i1="06" i2="3" l="ENG"><s0>Star models</s0>
<s5>31</s5>
</fC03>
<fC03 i1="07" i2="3" l="FRE"><s0>Evolution stellaire</s0>
<s5>32</s5>
</fC03>
<fC03 i1="07" i2="3" l="ENG"><s0>Stellar evolution</s0>
<s5>32</s5>
</fC03>
<fN21><s1>325</s1>
</fN21>
<fN44 i1="01"><s1>OTO</s1>
</fN44>
<fN82><s1>OTO</s1>
</fN82>
</pA>
</standard>
</inist>
</record>
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