Reference : Modelling a high-mass red giant observed by CoRoT
Scientific journals : Article
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/111305
Modelling a high-mass red giant observed by CoRoT
English
Baudin, F. [Institut d'Astrophysique Spatiale, UMR8617, CNRS, Université Paris XI, Bâtiment 121, 91405, Orsay Cedex, France]
Barban, C. [LESIA, UMR8109, CNRS, Université P. et M. Curie, Université D. Diderot, Observatoire de Paris, 92195, Meudon Cedex, France]
Goupil, M. J. [LESIA, UMR8109, CNRS, Université P. et M. Curie, Université D. Diderot, Observatoire de Paris, 92195, Meudon Cedex, France]
Samadi, R. [LESIA, UMR8109, CNRS, Université P. et M. Curie, Université D. Diderot, Observatoire de Paris, 92195, Meudon Cedex, France]
Lebreton, Y. [GEPI, UMR8111, CNRS, Université D. Diderot, Observatoire de Paris, 92195, Meudon Cedex, France]
Bruntt, H. [LESIA, UMR8109, CNRS, Université P. et M. Curie, Université D. Diderot, Observatoire de Paris, 92195, Meudon Cedex, France]
Morel, Thierry mailto [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Groupe d'astrophysique des hautes énergies (GAPHE)]
Lefèvre, L. [LESIA, UMR8109, CNRS, Université P. et M. Curie, Université D. Diderot, Observatoire de Paris, 92195, Meudon Cedex, France]
Michel, Etienne [> > > >]
Mosser, B. [LESIA, UMR8109, CNRS, Université P. et M. Curie, Université D. Diderot, Observatoire de Paris, 92195, Meudon Cedex, France]
Carrier, F. [Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Celestijnenlaan 200 B, 3001, Hervelee, Belgium]
De Ridder, J. [Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Celestijnenlaan 200 B, 3001, Hervelee, Belgium]
Hatzes, A. [Thüringer Landessternwarte, 07778, Tautenburg, Germany]
Hekker, S. [School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham, B15 2TT, UK; Astronomical Institute "Anton Pannekoek", University of Amsterdam, Science Park 904, 1098 XH, Amsterdam, The Netherlands]
Kallinger, T. [Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Celestijnenlaan 200 B, 3001, Hervelee, Belgium]
Auvergne, M. [LESIA, UMR8109, CNRS, Université P. et M. Curie, Université D. Diderot, Observatoire de Paris, 92195, Meudon Cedex, France]
Baglin, A. [LESIA, UMR8109, CNRS, Université P. et M. Curie, Université D. Diderot, Observatoire de Paris, 92195, Meudon Cedex, France]
Catala, C. [LESIA, UMR8109, CNRS, Université P. et M. Curie, Université D. Diderot, Observatoire de Paris, 92195, Meudon Cedex, France]
1-Feb-2012
Astronomy and Astrophysics
EDP Sciences
538
73
Yes (verified by ORBi)
International
0004-6361
1432-0746
Les Ulis
France
[en] stars: oscillations ; stars: interiors ; asteroseismology ; stars: individual: HR 2582 ; stars: individual: HD 50890 ; stars: individual: HIP 33243
[en] Context. The advent of space-borne photometers such as CoRoT and Kepler has opened up new fields in asteroseismology. This is especially true for red giants as only a few of these stars were known to oscillate with small amplitude, solar-like oscillations before the launch of CoRoT. <BR /> Aims: The G6 giant HR 2582 (HD 50890) was observed by CoRoT for approximately 55 days. We present here the analysis of its light curve and the characterisation of the star using different observables, such as its location in the Hertzsprung-Russell diagram and seismic observables. <BR /> Methods: Mode frequencies are extracted from the observed Fourier spectrum of the light curve. Numerical stellar models are then computed to determine the characteristics of the star (mass, age, etc.) from the comparison with observational constraints. <BR /> Results: We provide evidence for the presence of solar-like oscillations at low frequency, between 10 and 20 μHz, with a regular spacing of (1.7 ± 0.1) μHz between consecutive radial orders. Only radial modes are clearly visible. From the models compatible with the observational constraints used here, We find that HR 2582 (HD 50890) is a massive star with a mass in the range (3-5 M[SUB]&sun;[/SUB]), clearly above the red clump. It oscillates with rather low radial order (n = 5-12) modes. Its evolutionary stage cannot be determined with precision: the star could be on the ascending red giant branch (hydrogen shell burning) with an age of approximately 155 Myr or in a later phase (helium burning). In order to obtain a reasonable helium amount, the metallicity of the star must be quite subsolar. Our best models are obtained with a mixing length significantly smaller than that obtained for the Sun with the same physical description (except overshoot). The amount of core overshoot during the main-sequence phase is found to be mild, of the order of 0.1 H[SUB]p[/SUB]. <BR /> Conclusions: HR 2582 (HD 50890) is an interesting case as only a few massive stars can be observed due to their rapid evolution compared to less massive red giants. HR 2582 (HD 50890) is also one of the few cases that can be used to validate the scaling relations for massive red giants stars and its sensitivity to the physics of the star. The CoRoT space mission, launched on 2006 December 27, was developed and is operated by the CNES with participation of the Science Programs of ESA; ESA's RSSD, Austria, Belgium, Brazil, Germany and Spain.
http://hdl.handle.net/2268/111305
10.1051/0004-6361/201116967
http://adsabs.harvard.edu/abs/2012A%26A...538A..73B
http://de.arxiv.org/abs/1111.6543

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