AustralieFrV1, Main, Exploration, bibRecord, 005900

Spin down of the core rotation in red giants

Identifieur interne : 005900 ( Main/Exploration ); précédent : 005899; suivant : 005901

Spin down of the core rotation in red giants

Auteurs : B. Mosser [France] ; M. J. Goupil [France] ; K. Belkacem [France] ; J. P. Marques [Allemagne] ; P. G. Beck [Belgique] ; S. Bloemen [Belgique] ; J. De Ridder [Belgique] ; C. Barban [France] ; S. Deheuvels [États-Unis] ; Y. Elsworth [Royaume-Uni] ; S. Hekker [Royaume-Uni, Pays-Bas] ; T. Kallinger [Belgique] ; R. M. Ouazzani [France, Belgique] ; M. Pinsonneault [États-Unis] ; R. Samadi [France] ; D. Stello [Australie] ; R. A. Garcia [France] ; T. C. Klaus [États-Unis] ; J. Li [États-Unis] ; S. Mathur [États-Unis] ; R. L. Morris [États-Unis]

Source :

Astronomy and astrophysics : (Berlin. Print) [ 0004-6361 ] ; 2012.

RBID : Pascal:13-0063952

Descripteurs français

Pascal (Inist)
- Géante rouge, Série temporelle, Paramètre physique, Astéroséismologie, Evolution stellaire, Rotation stellaire, Etoile rouge, Moment cinétique, Masse stellaire, Rotation lente, Naine blanche, Etoile type avancé.

English descriptors

KwdEn :
- Angular momentum, Astroseismology, Late type stars, Physical parameter, Red giant stars, Red stars, Slow rotation, Stellar evolution, Stellar mass, Stellar rotation, Time series, White dwarf stars.

Abstract

Context. The space mission Kepler provides us with long and uninterrupted photometric time series of red giants. We are now able to probe the rotational behaviour in their deep interiors using the observations of mixed modes. Aims. We aim to measure the rotational splittings in red giants and to derive scaling relations for rotation related to seismic and fundamental stellar parameters. Methods. We have developed a dedicated method for automated measurements of the rotational splittings in a large number of red giants. Ensemble asteroseismology, namely the examination of a large number of red giants at different stages of their evolution, allows us to derive global information on stellar evolution. Results. We have measured rotational splittings in a sample of about 300 red giants. We have also shown that these splittings are dominated by the core rotation. Under the assumption that a linear analysis can provide the rotational splitting, we observe a small increase of the core rotation of stars ascending the red giant branch. Alternatively, an important slow down is observed for red-clump stars compared to the red giant branch. We also show that, at fixed stellar radius, the specific angular momentum increases with increasing stellar mass. Conclusions. Ensemble asteroseismology indicates what has been indirectly suspected for a while: our interpretation of the observed rotational splittings leads to the conclusion that the mean core rotation significantly slows down during the red giant phase. The slow-down occurs in the last stages of the red giant branch. This spinning down explains, for instance, the long rotation periods measured in white dwarfs.

Affiliations:

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Le document en format XML

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</affiliation>
</author>
<author><name sortKey="Belkacem, K" sort="Belkacem, K" uniqKey="Belkacem K" first="K." last="Belkacem">K. Belkacem</name>
<affiliation wicri:level="4"><inist:fA14 i1="01"><s1>LESIA, CNRS, Université Pierre et Marie Curie, Université Denis Diderot, Observatoire de Paris</s1>
<s2>92195 Meudon</s2>
<s3>FRA</s3>
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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>
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</placeName>
</affiliation>
</author>
<author><name sortKey="Marques, J P" sort="Marques, J P" uniqKey="Marques J" first="J. P." last="Marques">J. P. Marques</name>
<affiliation wicri:level="3"><inist:fA14 i1="02"><s1>Georg-August-Universitat Göttingen, Institut für Astrophysik, Friedrich-Hund-Platz 1</s1>
<s2>37077 Göttingen</s2>
<s3>DEU</s3>
<sZ>4 aut.</sZ>
</inist:fA14>
<country>Allemagne</country>
<placeName><region type="land" nuts="2">Basse-Saxe</region>
<settlement type="city">Göttingen</settlement>
</placeName>
</affiliation>
</author>
<author><name sortKey="Beck, P G" sort="Beck, P G" uniqKey="Beck P" first="P. G." last="Beck">P. G. Beck</name>
<affiliation wicri:level="3"><inist:fA14 i1="03"><s1>Instituut voor Sterrenkunde, K. U. Leuven, Celestijnenlaan 200D</s1>
<s2>3001 Leuven</s2>
<s3>BEL</s3>
<sZ>5 aut.</sZ>
<sZ>6 aut.</sZ>
<sZ>7 aut.</sZ>
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<country>Belgique</country>
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<settlement type="city">Louvain</settlement>
</placeName>
</affiliation>
</author>
<author><name sortKey="Bloemen, S" sort="Bloemen, S" uniqKey="Bloemen S" first="S." last="Bloemen">S. Bloemen</name>
<affiliation wicri:level="3"><inist:fA14 i1="03"><s1>Instituut voor Sterrenkunde, K. U. Leuven, Celestijnenlaan 200D</s1>
<s2>3001 Leuven</s2>
<s3>BEL</s3>
<sZ>5 aut.</sZ>
<sZ>6 aut.</sZ>
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<country>Belgique</country>
<placeName><region type="province" nuts="2">Province du Brabant flamand</region>
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<settlement type="city">Louvain</settlement>
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</affiliation>
</author>
<author><name sortKey="De Ridder, J" sort="De Ridder, J" uniqKey="De Ridder J" first="J." last="De Ridder">J. De Ridder</name>
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<s2>3001 Leuven</s2>
<s3>BEL</s3>
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<sZ>7 aut.</sZ>
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<country>Belgique</country>
<placeName><region type="province" nuts="2">Province du Brabant flamand</region>
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<settlement type="city">Louvain</settlement>
</placeName>
</affiliation>
</author>
<author><name sortKey="Barban, C" sort="Barban, C" uniqKey="Barban C" first="C." last="Barban">C. Barban</name>
<affiliation wicri:level="4"><inist:fA14 i1="01"><s1>LESIA, CNRS, Université Pierre et Marie Curie, Université Denis Diderot, Observatoire de Paris</s1>
<s2>92195 Meudon</s2>
<s3>FRA</s3>
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<sZ>8 aut.</sZ>
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<sZ>15 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>
</placeName>
</affiliation>
</author>
<author><name sortKey="Deheuvels, S" sort="Deheuvels, S" uniqKey="Deheuvels S" first="S." last="Deheuvels">S. Deheuvels</name>
<affiliation wicri:level="1"><inist:fA14 i1="04"><s1>Department of Astronomy, Yale University, PO Box 208101</s1>
<s2>New Haven, CT 06520-8101</s2>
<s3>USA</s3>
<sZ>9 aut.</sZ>
</inist:fA14>
<country>États-Unis</country>
<wicri:noRegion>New Haven, CT 06520-8101</wicri:noRegion>
</affiliation>
</author>
<author><name sortKey="Elsworth, Y" sort="Elsworth, Y" uniqKey="Elsworth Y" first="Y." last="Elsworth">Y. Elsworth</name>
<affiliation wicri:level="4"><inist:fA14 i1="05"><s1>School of Physics and Astronomy, University of Birmingham, Edgbaston</s1>
<s2>Birmingham B 15 2TT</s2>
<s3>GBR</s3>
<sZ>10 aut.</sZ>
<sZ>11 aut.</sZ>
</inist:fA14>
<country>Royaume-Uni</country>
<wicri:noRegion>Birmingham B 15 2TT</wicri:noRegion>
<orgName type="university">Université de Birmingham</orgName>
<placeName><settlement type="city">Birmingham</settlement>
<region type="country">Angleterre</region>
<region type="région" nuts="1">Midlands de l'Ouest</region>
</placeName>
</affiliation>
</author>
<author><name sortKey="Hekker, S" sort="Hekker, S" uniqKey="Hekker S" first="S." last="Hekker">S. Hekker</name>
<affiliation wicri:level="4"><inist:fA14 i1="05"><s1>School of Physics and Astronomy, University of Birmingham, Edgbaston</s1>
<s2>Birmingham B 15 2TT</s2>
<s3>GBR</s3>
<sZ>10 aut.</sZ>
<sZ>11 aut.</sZ>
</inist:fA14>
<country>Royaume-Uni</country>
<wicri:noRegion>Birmingham B 15 2TT</wicri:noRegion>
<orgName type="university">Université de Birmingham</orgName>
<placeName><settlement type="city">Birmingham</settlement>
<region type="country">Angleterre</region>
<region type="région" nuts="1">Midlands de l'Ouest</region>
</placeName>
</affiliation>
<affiliation wicri:level="4"><inist:fA14 i1="06"><s1>Astronomical Institute 'Anton Pannekoek', University of Amsterdam, Science Park 904</s1>
<s2>1098 XH Amsterdam</s2>
<s3>NLD</s3>
<sZ>11 aut.</sZ>
</inist:fA14>
<country>Pays-Bas</country>
<wicri:noRegion>1098 XH Amsterdam</wicri:noRegion>
<orgName type="university">Université d'Amsterdam</orgName>
<placeName><settlement type="city">Amsterdam</settlement>
<region>Hollande-Septentrionale</region>
</placeName>
</affiliation>
</author>
<author><name sortKey="Kallinger, T" sort="Kallinger, T" uniqKey="Kallinger T" first="T." last="Kallinger">T. Kallinger</name>
<affiliation wicri:level="3"><inist:fA14 i1="03"><s1>Instituut voor Sterrenkunde, K. U. Leuven, Celestijnenlaan 200D</s1>
<s2>3001 Leuven</s2>
<s3>BEL</s3>
<sZ>5 aut.</sZ>
<sZ>6 aut.</sZ>
<sZ>7 aut.</sZ>
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</inist:fA14>
<country>Belgique</country>
<placeName><region type="province" nuts="2">Province du Brabant flamand</region>
<settlement type="town">Heverlee</settlement>
<settlement type="city">Louvain</settlement>
</placeName>
</affiliation>
</author>
<author><name sortKey="Ouazzani, R M" sort="Ouazzani, R M" uniqKey="Ouazzani R" first="R. M." last="Ouazzani">R. M. Ouazzani</name>
<affiliation wicri:level="4"><inist:fA14 i1="01"><s1>LESIA, CNRS, Université Pierre et Marie Curie, Université Denis Diderot, Observatoire de Paris</s1>
<s2>92195 Meudon</s2>
<s3>FRA</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
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<sZ>8 aut.</sZ>
<sZ>13 aut.</sZ>
<sZ>15 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>
<affiliation wicri:level="4"><inist:fA14 i1="07"><s1>Institut d'Astrophysique et de Géophysique de l'Université de Liege, Allée du 6 Août 17</s1>
<s2>4000 Liege</s2>
<s3>BEL</s3>
<sZ>13 aut.</sZ>
</inist:fA14>
<country>Belgique</country>
<placeName><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>
</affiliation>
</author>
<author><name sortKey="Pinsonneault, M" sort="Pinsonneault, M" uniqKey="Pinsonneault M" first="M." last="Pinsonneault">M. Pinsonneault</name>
<affiliation wicri:level="1"><inist:fA14 i1="08"><s1>Department of Astronomy, The Ohio State University</s1>
<s2>Columbus, OH 43210</s2>
<s3>USA</s3>
<sZ>14 aut.</sZ>
</inist:fA14>
<country>États-Unis</country>
<wicri:noRegion>Columbus, OH 43210</wicri:noRegion>
</affiliation>
</author>
<author><name sortKey="Samadi, R" sort="Samadi, R" uniqKey="Samadi R" first="R." last="Samadi">R. Samadi</name>
<affiliation wicri:level="4"><inist:fA14 i1="01"><s1>LESIA, CNRS, Université Pierre et Marie Curie, Université Denis Diderot, Observatoire de Paris</s1>
<s2>92195 Meudon</s2>
<s3>FRA</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
<sZ>8 aut.</sZ>
<sZ>13 aut.</sZ>
<sZ>15 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="Stello, D" sort="Stello, D" uniqKey="Stello D" first="D." last="Stello">D. Stello</name>
<affiliation wicri:level="4"><inist:fA14 i1="09"><s1>Sydney Institute for Astronomy, School of Physics, University of Sydney</s1>
<s2>NSW 2006</s2>
<s3>AUS</s3>
<sZ>16 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="Garcia, R A" sort="Garcia, R A" uniqKey="Garcia R" first="R. A." last="Garcia">R. A. Garcia</name>
<affiliation wicri:level="3"><inist:fA14 i1="10"><s1>Laboratoire AIM, CEA/DSM CNRS - Université Denis Diderot IRFU/SAp</s1>
<s2>91191 Gif-sur-Yvette</s2>
<s3>FRA</s3>
<sZ>17 aut.</sZ>
</inist:fA14>
<country>France</country>
<placeName><region type="region" nuts="2">Île-de-France</region>
<settlement type="city">Gif-sur-Yvette</settlement>
</placeName>
</affiliation>
</author>
<author><name sortKey="Klaus, T C" sort="Klaus, T C" uniqKey="Klaus T" first="T. C." last="Klaus">T. C. Klaus</name>
<affiliation wicri:level="1"><inist:fA14 i1="11"><s1>Orbital Sciences Corporation/NASA Ames Research Center</s1>
<s2>Moffett Field, CA 94035</s2>
<s3>USA</s3>
<sZ>18 aut.</sZ>
</inist:fA14>
<country>États-Unis</country>
<wicri:noRegion>Orbital Sciences Corporation/NASA Ames Research Center</wicri:noRegion>
</affiliation>
</author>
<author><name sortKey="Li, J" sort="Li, J" uniqKey="Li J" first="J." last="Li">J. Li</name>
<affiliation wicri:level="1"><inist:fA14 i1="12"><s1>SETI Institute/NASA Ames Research Center</s1>
<s2>Moffett Field, CA 94035</s2>
<s3>USA</s3>
<sZ>19 aut.</sZ>
<sZ>21 aut.</sZ>
</inist:fA14>
<country>États-Unis</country>
<wicri:noRegion>SETI Institute/NASA Ames Research Center</wicri:noRegion>
</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="13"><s1>High Altitude Observatory, NCAR, PO Box 3000</s1>
<s2>Boulder, CO 80307</s2>
<s3>USA</s3>
<sZ>20 aut.</sZ>
</inist:fA14>
<country>États-Unis</country>
<wicri:noRegion>Boulder, CO 80307</wicri:noRegion>
</affiliation>
</author>
<author><name sortKey="Morris, R L" sort="Morris, R L" uniqKey="Morris R" first="R. L." last="Morris">R. L. Morris</name>
<affiliation wicri:level="1"><inist:fA14 i1="12"><s1>SETI Institute/NASA Ames Research Center</s1>
<s2>Moffett Field, CA 94035</s2>
<s3>USA</s3>
<sZ>19 aut.</sZ>
<sZ>21 aut.</sZ>
</inist:fA14>
<country>États-Unis</country>
<wicri:noRegion>SETI Institute/NASA Ames Research Center</wicri:noRegion>
</affiliation>
</author>
</analytic>
<series><title level="j" type="main">Astronomy and astrophysics : (Berlin. Print)</title>
<title level="j" type="abbreviated">Astron. astrophys. : (Berl., Print)</title>
<idno type="ISSN">0004-6361</idno>
<imprint><date when="2012">2012</date>
</imprint>
</series>
</biblStruct>
</sourceDesc>
<seriesStmt><title level="j" type="main">Astronomy and astrophysics : (Berlin. Print)</title>
<title level="j" type="abbreviated">Astron. astrophys. : (Berl., Print)</title>
<idno type="ISSN">0004-6361</idno>
</seriesStmt>
</fileDesc>
<profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>Angular momentum</term>
<term>Astroseismology</term>
<term>Late type stars</term>
<term>Physical parameter</term>
<term>Red giant stars</term>
<term>Red stars</term>
<term>Slow rotation</term>
<term>Stellar evolution</term>
<term>Stellar mass</term>
<term>Stellar rotation</term>
<term>Time series</term>
<term>White dwarf stars</term>
</keywords>
<keywords scheme="Pascal" xml:lang="fr"><term>Géante rouge</term>
<term>Série temporelle</term>
<term>Paramètre physique</term>
<term>Astéroséismologie</term>
<term>Evolution stellaire</term>
<term>Rotation stellaire</term>
<term>Etoile rouge</term>
<term>Moment cinétique</term>
<term>Masse stellaire</term>
<term>Rotation lente</term>
<term>Naine blanche</term>
<term>Etoile type avancé</term>
</keywords>
</textClass>
</profileDesc>
</teiHeader>
<front><div type="abstract" xml:lang="en">Context. The space mission Kepler provides us with long and uninterrupted photometric time series of red giants. We are now able to probe the rotational behaviour in their deep interiors using the observations of mixed modes. Aims. We aim to measure the rotational splittings in red giants and to derive scaling relations for rotation related to seismic and fundamental stellar parameters. Methods. We have developed a dedicated method for automated measurements of the rotational splittings in a large number of red giants. Ensemble asteroseismology, namely the examination of a large number of red giants at different stages of their evolution, allows us to derive global information on stellar evolution. Results. We have measured rotational splittings in a sample of about 300 red giants. We have also shown that these splittings are dominated by the core rotation. Under the assumption that a linear analysis can provide the rotational splitting, we observe a small increase of the core rotation of stars ascending the red giant branch. Alternatively, an important slow down is observed for red-clump stars compared to the red giant branch. We also show that, at fixed stellar radius, the specific angular momentum increases with increasing stellar mass. Conclusions. Ensemble asteroseismology indicates what has been indirectly suspected for a while: our interpretation of the observed rotational splittings leads to the conclusion that the mean core rotation significantly slows down during the red giant phase. The slow-down occurs in the last stages of the red giant branch. This spinning down explains, for instance, the long rotation periods measured in white dwarfs.</div>
</front>
</TEI>
<affiliations><list><country><li>Allemagne</li>
<li>Australie</li>
<li>Belgique</li>
<li>France</li>
<li>Pays-Bas</li>
<li>Royaume-Uni</li>
<li>États-Unis</li>
</country>
<region><li>Angleterre</li>
<li>Basse-Saxe</li>
<li>Hollande-Septentrionale</li>
<li>Midlands de l'Ouest</li>
<li>Nouvelle-Galles du Sud</li>
<li>Province de Liège</li>
<li>Province du Brabant flamand</li>
<li>Île-de-France</li>
</region>
<settlement><li>Amsterdam</li>
<li>Birmingham</li>
<li>Gif-sur-Yvette</li>
<li>Göttingen</li>
<li>Heverlee</li>
<li>Liège</li>
<li>Louvain</li>
<li>Meudon</li>
<li>Paris</li>
<li>Sydney</li>
</settlement>
<orgName><li>Université Pierre-et-Marie-Curie</li>
<li>Université d'Amsterdam</li>
<li>Université de Birmingham</li>
<li>Université de Liège</li>
<li>Université de Sydney</li>
</orgName>
</list>
<tree><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>
<name sortKey="Barban, C" sort="Barban, C" uniqKey="Barban C" first="C." last="Barban">C. Barban</name>
<name sortKey="Belkacem, K" sort="Belkacem, K" uniqKey="Belkacem K" first="K." last="Belkacem">K. Belkacem</name>
<name sortKey="Garcia, R A" sort="Garcia, R A" uniqKey="Garcia R" first="R. A." last="Garcia">R. A. Garcia</name>
<name sortKey="Goupil, M J" sort="Goupil, M J" uniqKey="Goupil M" first="M. J." last="Goupil">M. J. Goupil</name>
<name sortKey="Ouazzani, R M" sort="Ouazzani, R M" uniqKey="Ouazzani R" first="R. M." last="Ouazzani">R. M. Ouazzani</name>
<name sortKey="Samadi, R" sort="Samadi, R" uniqKey="Samadi R" first="R." last="Samadi">R. Samadi</name>
</country>
<country name="Allemagne"><region name="Basse-Saxe"><name sortKey="Marques, J P" sort="Marques, J P" uniqKey="Marques J" first="J. P." last="Marques">J. P. Marques</name>
</region>
</country>
<country name="Belgique"><region name="Province du Brabant flamand"><name sortKey="Beck, P G" sort="Beck, P G" uniqKey="Beck P" first="P. G." last="Beck">P. G. Beck</name>
</region>
<name sortKey="Bloemen, S" sort="Bloemen, S" uniqKey="Bloemen S" first="S." last="Bloemen">S. Bloemen</name>
<name sortKey="De Ridder, J" sort="De Ridder, J" uniqKey="De Ridder J" first="J." last="De Ridder">J. De Ridder</name>
<name sortKey="Kallinger, T" sort="Kallinger, T" uniqKey="Kallinger T" first="T." last="Kallinger">T. Kallinger</name>
<name sortKey="Ouazzani, R M" sort="Ouazzani, R M" uniqKey="Ouazzani R" first="R. M." last="Ouazzani">R. M. Ouazzani</name>
</country>
<country name="États-Unis"><noRegion><name sortKey="Deheuvels, S" sort="Deheuvels, S" uniqKey="Deheuvels S" first="S." last="Deheuvels">S. Deheuvels</name>
</noRegion>
<name sortKey="Klaus, T C" sort="Klaus, T C" uniqKey="Klaus T" first="T. C." last="Klaus">T. C. Klaus</name>
<name sortKey="Li, J" sort="Li, J" uniqKey="Li J" first="J." last="Li">J. Li</name>
<name sortKey="Mathur, S" sort="Mathur, S" uniqKey="Mathur S" first="S." last="Mathur">S. Mathur</name>
<name sortKey="Morris, R L" sort="Morris, R L" uniqKey="Morris R" first="R. L." last="Morris">R. L. Morris</name>
<name sortKey="Pinsonneault, M" sort="Pinsonneault, M" uniqKey="Pinsonneault M" first="M." last="Pinsonneault">M. Pinsonneault</name>
</country>
<country name="Royaume-Uni"><region name="Angleterre"><name sortKey="Elsworth, Y" sort="Elsworth, Y" uniqKey="Elsworth Y" first="Y." last="Elsworth">Y. Elsworth</name>
</region>
<name sortKey="Hekker, S" sort="Hekker, S" uniqKey="Hekker S" first="S." last="Hekker">S. Hekker</name>
</country>
<country name="Pays-Bas"><region name="Hollande-Septentrionale"><name sortKey="Hekker, S" sort="Hekker, S" uniqKey="Hekker S" first="S." last="Hekker">S. Hekker</name>
</region>
</country>
<country name="Australie"><region name="Nouvelle-Galles du Sud"><name sortKey="Stello, D" sort="Stello, D" uniqKey="Stello D" first="D." last="Stello">D. Stello</name>
</region>
</country>
</tree>
</affiliations>
</record>

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{{Explor lien
   |wiki=    Wicri/Asie
   |area=    AustralieFrV1
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   |étape=   Exploration
   |type=    RBID
   |clé=     Pascal:13-0063952
   |texte=   Spin down of the core rotation in red giants
}}

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	Serveur d'exploration sur les relations entre la France et l'Australie
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Serveur d'exploration sur les relations entre la France et l'Australie

Spin down of the core rotation in red giants

Spin down of the core rotation in red giants

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