Article (Scientific journals)
Seismic analysis of HD 43587Aa, a solar-like oscillator in a multiple system
Boumier, P.; Benomar, O.; Baudin, F. et al.
2014In Astronomy and Astrophysics, 564, p. 34
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Keywords :
asteroseismology; stars: individual: HD 43587Aa; binaries: general; stars: solar-type; methods: data analysis
Abstract :
[en] Context. The object HD 43587Aa is a G0V star observed during the 145-day LRa03 run of the COnvection, ROtation and planetary Transits space mission (CoRoT), for which complementary High Accuracy Radial velocity Planet Searcher (HARPS) spectra with S/N > 300 were also obtained. Its visual magnitude is 5.71, and its effective temperature is close to 5950 K. It has a known companion in a highly eccentric orbit and is also coupled with two more distant companions. <BR /> Aims: We undertake a preliminary investigation of the internal structure of HD 43587Aa. <BR /> Methods: We carried out a seismic analysis of the star, using maximum likelihood estimators and Markov chain Monte Carlo methods. <BR /> Results: We established the first table of the eigenmode frequencies, widths, and heights for HD 43587Aa. The star appears to have a mass and a radius slightly larger than the Sun, and is slightly older (5.6 Gyr). Two scenarios are suggested for the geometry of the star: either its inclination angle is very low, or the rotation velocity of the star is very low. <BR /> Conclusions: A more detailed study of the rotation and of the magnetic and chromospheric activity for this star is needed, and will be the subject of a further study. New high resolution spectrometric observations should be performed for at least several months in duration.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Boumier, P.;  Institut d'Astrophysique Spatiale, CNRS, Université Paris Sud, UMR 8617, 91405, Orsay Cedex, France
Benomar, O.;  Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney, NSW, 2006, Sydney, Australia
Baudin, F.;  Institut d'Astrophysique Spatiale, CNRS, Université Paris Sud, UMR 8617, 91405, Orsay Cedex, France
Verner, G.;  Astronomy Unit, Queen Mary, University of London, Mile End Road, London, E1 4NS, UK
Appourchaux, T.;  Institut d'Astrophysique Spatiale, CNRS, Université Paris Sud, UMR 8617, 91405, Orsay Cedex, France
Lebreton, Y.;  GEPI, Observatoire de Paris, CNRS UMR 8111, 92195, Meudon, France ; Institut de Physique de Rennes, Université de Rennes 1, CNRS UMR 6251, 35042, Rennes, France
Gaulme, P.;  New Mexico State University, Department of Astronomy, PO Box 30001, MSC 4500, Las Cruces, NM, USA
Chaplin, W.;  School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham, B15 2TT, UK
García, R. A.;  Laboratoire AIM, CEA/DSM-CNRS, Université Paris 7 Diderot, IRFU/Sap, Centre de Saclay, 91191, Gif-sur-Yvette, France
Hekker, S.;  Astronomical Institute "Anton Pannekoek", University of Amsterdam, Science Park 904, 1098 XH, Amsterdam, the Netherlands ; Max-Planck-Institut für Sonnensystemforschung, Justus-von-Liebig-Weg 3, 37077, Göttingen, Germany
Regulo, C.;  Instituto de Astrofísica de Canarias, 38205 La Laguna, Tenerife, Spain ; Universidad de La Laguna, Dpto de Astrofísica, 38206 La Laguna, Tenerife, Spain
Salabert, D.;  Université de Nice Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, BP 4229, 06304, Nice Cedex 4, France
Stahn, T.;  Institut für Astrophysik, Georg-August-Universität Göttingen, 37077, Göttingen, Germany
Elsworth, Y.;  School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham, B15 2TT, UK
Gizon, L.;  Max-Planck-Institut für Sonnensystemforschung, Justus-von-Liebig-Weg 3, 37077, Göttingen, Germany ; Institut für Astrophysik, Georg-August-Universität Göttingen, 37077, Göttingen, Germany
Hall, M.;  Astronomy Unit, Queen Mary, University of London, Mile End Road, London, E1 4NS, UK
Mathur, S.;  High Altitude Observatory, NCAR, PO Box 3000, Boulder, CO, 80307, USA ; Space Science Institute, 4750 Walnut Street Suite 205, Boulder, CO, 80301, USA
Michel, Eric
Morel, Thierry  ;  Université de Liège - ULiège > Groupe d'astrophysique des hautes énergies (GAPHE)
Mosser, B.;  LESIA, Observatoire de Paris, CNRS, Université Paris 6, Université Paris 7, UMR 8109, 92195, Meudon Cedex, France
Poretti, E.;  INAF - Osservatorio Astronomico di Brera, via E. Bianchi 46, 23807, Merate, Italy
Rainer, M.;  INAF - Osservatorio Astronomico di Brera, via E. Bianchi 46, 23807, Merate, Italy
Roxburgh, I.;  Astronomy Unit, Queen Mary, University of London, Mile End Road, London, E1 4NS, UK
do Nascimento, J.-D.;  Institut d'Astrophysique Spatiale, CNRS, Université Paris Sud, UMR 8617, 91405, Orsay Cedex, France ; Depart. de Física Teórica e Experimental, Univ. Federal do Rio Grande do Norte, CEP 59072-970, Natal, RN, Brazil
Samadi, R.;  LESIA, Observatoire de Paris, CNRS, Université Paris 6, Université Paris 7, UMR 8109, 92195, Meudon Cedex, France
Auvergne, M.;  LESIA, Observatoire de Paris, CNRS, Université Paris 6, Université Paris 7, UMR 8109, 92195, Meudon Cedex, France
Chaintreuil, S.;  LESIA, Observatoire de Paris, CNRS, Université Paris 6, Université Paris 7, UMR 8109, 92195, Meudon Cedex, France
Baglin, A.;  LESIA, Observatoire de Paris, CNRS, Université Paris 6, Université Paris 7, UMR 8109, 92195, Meudon Cedex, France
Catala, C.;  LESIA, Observatoire de Paris, CNRS, Université Paris 6, Université Paris 7, UMR 8109, 92195, Meudon Cedex, France)
More authors (19 more) Less
Language :
English
Title :
Seismic analysis of HD 43587Aa, a solar-like oscillator in a multiple system
Publication date :
01 April 2014
Journal title :
Astronomy and Astrophysics
ISSN :
0004-6361
eISSN :
1432-0746
Publisher :
EDP Sciences, Les Ulis, France
Volume :
564
Pages :
34
Peer reviewed :
Peer Reviewed verified by ORBi
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