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SOLAR-LIKE OSCILLATIONS IN LOW-LUMINOSITY RED GIANTS: FIRST RESULTS FROM KEPLER

Identifieur interne : 007564 ( Main/Curation ); précédent : 007563; suivant : 007565

SOLAR-LIKE OSCILLATIONS IN LOW-LUMINOSITY RED GIANTS: FIRST RESULTS FROM KEPLER

Auteurs : T. R. Bedding [Australie] ; D. Huber [Australie] ; D. Stello [Australie] ; Y. P. Elsworth [Royaume-Uni] ; S. Hekker [Royaume-Uni] ; T. Kallinger [Canada, Autriche] ; S. Mathur [Inde] ; B. Mosser [France] ; H. L. Preston [États-Unis, Afrique du Sud] ; J. Ballot [France] ; C. Barban [France] ; A. M. Broomhall [Royaume-Uni] ; D. L. Buzasi [États-Unis] ; W. J. Chaplin [Royaume-Uni] ; R. A. Garcia [France] ; M. Gruberbauer [Canada] ; S. J. Hale [Royaume-Uni] ; J. De Ridder [Belgique] ; S. Frandsen [Danemark] ; W. J. Borucki [États-Unis] ; T. Brown [États-Unis] ; J. Christensen-Dalsgaard [Danemark] ; R. L. Gilliland [États-Unis] ; J. M. Jenkins [États-Unis] ; H. Kjeldsen [Danemark] ; D. Koch [États-Unis] ; K. Belkacem [Belgique] ; L. Bildsten [États-Unis] ; H. Bruntt [France, Danemark] ; T. L. Campante [Danemark, Portugal] ; S. Deheuvels [France] ; A. Derekas [Australie, Hongrie] ; M.-A. Dupret [Belgique] ; M.-J. Goupil [France] ; A. Hatzes [Allemagne] ; G. Houdek [Autriche] ; M. J. Ireland [Australie] ; C. Jiang [République populaire de Chine] ; C. Karoff [Royaume-Uni] ; L. L. Kiss [Australie, Hongrie] ; Y. Lebreton [France] ; A. Miglio [Belgique] ; J. Montalban [Belgique] ; A. Noels [Belgique] ; I. W. Roxburgh [Royaume-Uni] ; V. Sangaralingam [Royaume-Uni] ; I. R. Stevens [Royaume-Uni] ; M. D. Suran [Roumanie] ; N. J. Tarrant [Royaume-Uni] ; A. Weiss

Source :

RBID : Pascal:11-0296982

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Abstract

We have measured solar-like oscillations in red giants using time-series photometry from the first 34 days of science operations of the Kepler Mission. The light curves, obtained with 30 minute sampling, reveal clear oscillations in a large sample of G and K giants, extending in luminosity from the red clump down to the bottom of the giant branch. We confirm a strong correlation between the large separation of the oscillations (Δv) and the frequency of maximum power (vmax). We focus on a sample of 50 low-luminosity stars (vmax > 100 μHz, L ? 30 L◦.) having high signal-to-noise ratios and showing the unambiguous signature of solar-like oscillations. These are H-shell-burning stars, whose oscillations should be valuable for testing models of stellar evolution and for constraining the star formation rate in the local disk.

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Pascal:11-0296982

Le document en format XML

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<sZ>32 aut.</sZ>
<sZ>40 aut.</sZ>
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<name sortKey="Hatzes, A" sort="Hatzes, A" uniqKey="Hatzes A" first="A." last="Hatzes">A. Hatzes</name>
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<orgName type="university">Université de Sydney</orgName>
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<name sortKey="Jiang, C" sort="Jiang, C" uniqKey="Jiang C" first="C." last="Jiang">C. Jiang</name>
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<s1>Department of Astronomy. Beijing Normal University</s1>
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<country>République populaire de Chine</country>
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<s1>Queen Mary University of London, Mile End Road</s1>
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<title xml:lang="en" level="a">SOLAR-LIKE OSCILLATIONS IN LOW-LUMINOSITY RED GIANTS: FIRST RESULTS FROM KEPLER</title>
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<settlement type="city">Paris</settlement>
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</affiliation>
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<s1>Danish AsteroSeismology Centre (DASC), Department of Physics and Astronomy, Aarhus University</s1>
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<name sortKey="Campante, T L" sort="Campante, T L" uniqKey="Campante T" first="T. L." last="Campante">T. L. Campante</name>
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<country>Portugal</country>
<wicri:noRegion>Centro de Astrofísica da Universidade do Porto. Rua das Estrelas</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Deheuvels, S" sort="Deheuvels, S" uniqKey="Deheuvels S" first="S." last="Deheuvels">S. Deheuvels</name>
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<sZ>31 aut.</sZ>
<sZ>34 aut.</sZ>
<sZ>41 aut.</sZ>
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<wicri:noRegion>Observatoire de Paris</wicri:noRegion>
<wicri:noRegion>92195 Meudon</wicri:noRegion>
<orgName type="university">Université Pierre-et-Marie-Curie</orgName>
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<settlement type="city">Paris</settlement>
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<sZ>40 aut.</sZ>
</inist:fA14>
<country>Hongrie</country>
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<name sortKey="Dupret, M A" sort="Dupret, M A" uniqKey="Dupret M" first="M.-A." last="Dupret">M.-A. Dupret</name>
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<region type="province" nuts="2">Province de Liège</region>
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<orgName type="university">Université de Liège</orgName>
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<name sortKey="Goupil, M J" sort="Goupil, M J" uniqKey="Goupil M" first="M.-J." last="Goupil">M.-J. Goupil</name>
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<wicri:noRegion>Observatoire de Paris</wicri:noRegion>
<wicri:noRegion>92195 Meudon</wicri:noRegion>
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<name sortKey="Hatzes, A" sort="Hatzes, A" uniqKey="Hatzes A" first="A." last="Hatzes">A. Hatzes</name>
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<s1>Thueringer Landessternwarte Tautenburg, Sternwarte 5</s1>
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<region type="land" nuts="2">Thuringe</region>
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<name sortKey="Houdek, G" sort="Houdek, G" uniqKey="Houdek G" first="G." last="Houdek">G. Houdek</name>
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<region type="land" nuts="2">Vienne (Autriche)</region>
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<name sortKey="Ireland, M J" sort="Ireland, M J" uniqKey="Ireland M" first="M. J." last="Ireland">M. J. Ireland</name>
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<inist:fA14 i1="01">
<s1>Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney</s1>
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<sZ>1 aut.</sZ>
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<country>Australie</country>
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<settlement type="city">Sydney</settlement>
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</placeName>
<orgName type="university">Université de Sydney</orgName>
</affiliation>
</author>
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<name sortKey="Jiang, C" sort="Jiang, C" uniqKey="Jiang C" first="C." last="Jiang">C. Jiang</name>
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<s1>Department of Astronomy. Beijing Normal University</s1>
<s3>CHN</s3>
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<country>République populaire de Chine</country>
<wicri:noRegion>Department of Astronomy. Beijing Normal University</wicri:noRegion>
</affiliation>
</author>
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<name sortKey="Karoff, C" sort="Karoff, C" uniqKey="Karoff C" first="C." last="Karoff">C. Karoff</name>
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<country>Royaume-Uni</country>
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<settlement type="city">Birmingham</settlement>
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<orgName type="university">Université de Birmingham</orgName>
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<name sortKey="Kiss, L L" sort="Kiss, L L" uniqKey="Kiss L" first="L. L." last="Kiss">L. L. Kiss</name>
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<settlement type="city">Sydney</settlement>
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</placeName>
<orgName type="university">Université de Sydney</orgName>
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<country>Hongrie</country>
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<name sortKey="Lebreton, Y" sort="Lebreton, Y" uniqKey="Lebreton Y" first="Y." last="Lebreton">Y. Lebreton</name>
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<s1>LESIA, CNRS, Université Pierre et Marie Curie, Université Denis, Diderot, Observatoire de Paris</s1>
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<sZ>8 aut.</sZ>
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<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>
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<name sortKey="Miglio, A" sort="Miglio, A" uniqKey="Miglio A" first="A." last="Miglio">A. Miglio</name>
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<country>Belgique</country>
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<region type="province" nuts="2">Province de Liège</region>
<settlement type="city">Liège</settlement>
<settlement type="city">Liège</settlement>
</placeName>
<orgName type="university">Université de Liège</orgName>
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<name sortKey="Montalban, J" sort="Montalban, J" uniqKey="Montalban J" first="J." last="Montalban">J. Montalban</name>
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<country>Belgique</country>
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<region type="province" nuts="2">Province de Liège</region>
<settlement type="city">Liège</settlement>
<settlement type="city">Liège</settlement>
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<orgName type="university">Université de Liège</orgName>
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<name sortKey="Noels, A" sort="Noels, A" uniqKey="Noels A" first="A." last="Noels">A. Noels</name>
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<s1>Institut d'Astrophysique et de Géophysique de l'Université de Liege, Allée du 6 Aout 17</s1>
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<country>Belgique</country>
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<region type="province" nuts="2">Province de Liège</region>
<settlement type="city">Liège</settlement>
<settlement type="city">Liège</settlement>
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<orgName type="university">Université de Liège</orgName>
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<name sortKey="Roxburgh, I W" sort="Roxburgh, I W" uniqKey="Roxburgh I" first="I. W." last="Roxburgh">I. W. Roxburgh</name>
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<s1>Queen Mary University of London, Mile End Road</s1>
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<country>Royaume-Uni</country>
<wicri:noRegion>London E1 4NS</wicri:noRegion>
<orgName type="university">Université de Londres</orgName>
<placeName>
<settlement type="city">Londres</settlement>
<region type="country">Angleterre</region>
<region type="région" nuts="1">Grand Londres</region>
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</affiliation>
</author>
<author>
<name sortKey="Sangaralingam, V" sort="Sangaralingam, V" uniqKey="Sangaralingam V" first="V." last="Sangaralingam">V. Sangaralingam</name>
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<s1>School of Physics and Astronomy, University of Birmingham</s1>
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<orgName type="university">Université de Birmingham</orgName>
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<author>
<name sortKey="Stevens, I R" sort="Stevens, I R" uniqKey="Stevens I" first="I. R." last="Stevens">I. R. Stevens</name>
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<settlement type="city">Birmingham</settlement>
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<orgName type="university">Université de Birmingham</orgName>
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<name sortKey="Suran, M D" sort="Suran, M D" uniqKey="Suran M" first="M. D." last="Suran">M. D. Suran</name>
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<country>Roumanie</country>
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<author>
<name sortKey="Tarrant, N J" sort="Tarrant, N J" uniqKey="Tarrant N" first="N. J." last="Tarrant">N. J. Tarrant</name>
<affiliation wicri:level="4">
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<s1>School of Physics and Astronomy, University of Birmingham</s1>
<s2>Birmingham B 15 2TT</s2>
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<placeName>
<settlement type="city">Birmingham</settlement>
<region type="country">Angleterre</region>
<region type="région" nuts="1">Midlands de l'Ouest</region>
</placeName>
<orgName type="university">Université de Birmingham</orgName>
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</author>
<author>
<name sortKey="Weiss, A" sort="Weiss, A" uniqKey="Weiss A" first="A." last="Weiss">A. Weiss</name>
</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="2010">2010</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>Formation rate</term>
<term>Light curves</term>
<term>Luminosity</term>
<term>Photometry</term>
<term>Red giant stars</term>
<term>Shell stars</term>
<term>Signal-to-noise ratio</term>
<term>Solar type star</term>
<term>Star burning</term>
<term>Star formation</term>
<term>Star models</term>
<term>Strong correlation</term>
<term>Sun</term>
<term>Time series</term>
</keywords>
<keywords scheme="Pascal" xml:lang="fr">
<term>Luminosité</term>
<term>Géante rouge</term>
<term>Série temporelle</term>
<term>Photométrie</term>
<term>Courbe lumière</term>
<term>Corrélation forte</term>
<term>Rapport signal bruit</term>
<term>Etoile enveloppe</term>
<term>Combustion stellaire</term>
<term>Modèle stellaire</term>
<term>Formation stellaire</term>
<term>Taux formation</term>
<term>Soleil</term>
<term>Etoile type solaire</term>
<term>Astéroséismologie</term>
</keywords>
</textClass>
</profileDesc>
</teiHeader>
<front>
<div type="abstract" xml:lang="en">We have measured solar-like oscillations in red giants using time-series photometry from the first 34 days of science operations of the Kepler Mission. The light curves, obtained with 30 minute sampling, reveal clear oscillations in a large sample of G and K giants, extending in luminosity from the red clump down to the bottom of the giant branch. We confirm a strong correlation between the large separation of the oscillations (Δv) and the frequency of maximum power (v
<sub>max</sub>
). We focus on a sample of 50 low-luminosity stars (v
<sub>max</sub>
> 100 μHz, L ? 30 L
<sub>◦.</sub>
) having high signal-to-noise ratios and showing the unambiguous signature of solar-like oscillations. These are H-shell-burning stars, whose oscillations should be valuable for testing models of stellar evolution and for constraining the star formation rate in the local disk.</div>
</front>
</TEI>
</record>

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