asteroseismology; stars: abundances; stars: fundamental parameters; stars: interiors; stars: solar-type; Astrophysics - Solar and Stellar Astrophysics
Abstract :
[en] Solar analogues are important stars to study for understanding the properties of the Sun. Combined with seismic and spectroscopic analysis, evolutionary modelling becomes a powerful method to characterize stellar intrinsic parameters, such as mass, radius, metallicity and age. However, these characteristics, relevant for other aspects of astrophysics or exoplanetary system physics, for example, are difficult to obtain with high precision and/or accuracy. The goal of this study is to characterize the two solar analogues, HD 42618 and HD 43587, observed by CoRoT. In particular, we aim to infer their precise mass, radius and age, using evolutionary modelling constrained by spectroscopic, photometric and seismic analysis. These stars show evidence of being older than the Sun but with a relatively large lithium abundance. We present the seismic analysis of HD 42618, and the modelling of the two solar analogues, HD 42618 and HD 43587 using the CESTAM stellar evolution code. Models were computed to reproduce the spectroscopic (effective temperature and metallicity) and seismic (mode frequency) data, and the luminosity of the stars, based on Gaia parallaxes. We infer very similar values of mass and radius for both stars compared with the literature, within the uncertainties, and we reproduce correctly the seismic constraints. The modelling shows that HD 42618 is slightly less massive and older than the Sun, and that HD 43587 is more massive and older than the Sun, in agreement with previous results. The use of chemical clocks improves the reliability of our age estimates.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Castro, M.; Departamento de Física, Universidade Federal do Rio Grande do Norte, CEP: 59072-970 Natal, RN, Brazil
Baudin, F.; Université Paris-Sud, CNRS, Institut d'Astrophysique Spatiale, UMR 8617, F-91405, Orsay Cedex, France
Benomar, O.; Center for Space Science, NYUAD Institute, New York University Abu Dhabi, PO Box 129188, Abu Dhabi, UAE ; Division of Solar and Plasma Astrophysics, NAOJ, Mitaka, Tokyo, Japan
Samadi, R.; LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, 5 place Jules Janssen, F-92195 Meudon, France
Morel, Thierry ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie
Barban, C.; LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, 5 place Jules Janssen, F-92195 Meudon, France
do Nascimento, J. D.; Departamento de Física, Universidade Federal do Rio Grande do Norte, CEP: 59072-970 Natal, RN, Brazil ; Université Paris-Sud, CNRS, Institut d'Astrophysique Spatiale, UMR 8617, F-91405, Orsay Cedex, France ; Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA
Lebreton, Y.; LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, 5 place Jules Janssen, F-92195 Meudon, France ; Université Rennes, CNRS, IPR (Institut de Physique de Rennes) - UMR 6251, F-35000 Rennes, France
Boumier, P.; Université Paris-Sud, CNRS, Institut d'Astrophysique Spatiale, UMR 8617, F-91405, Orsay Cedex, France
Marques, J. P.; Université Paris-Sud, CNRS, Institut d'Astrophysique Spatiale, UMR 8617, F-91405, Orsay Cedex, France
da Costa, J. S.; Escola de Ciência e Tecnologia, Universidade Federal do Rio Grande do Norte, CEP: 59072-970 Natal, RN, Brazil)
Language :
English
Title :
Modeling of two CoRoT solar analogues constrained by seismic and spectroscopic analysis
Asplund M., Grevesse N., Sauval A. J., Scott P., 2009, ARA&A, 47, 481
Baglin A., Auvergne M., Barge P., Deleuil M., Catala C., Michel E., Weiss W., CoRoT Team, 2006, in Fridlund M., Baglin A., Lochard J., Conroy L., eds, ESA Special Publication Vol. 1306, The CoRoT Mission Pre- Launch Status - Stellar Seismology and Planet Finding. ESA Publications, Noordwijk, p. 33
Baliunas S. L. et al., 1995, ApJ, 438, 269
Ballot J. et al., 2011, A&A, 530, A97
Barban C. et al., 2013, J. Phys.: Conf. Ser., 440, 012030
Baumann P., Ramírez I.,Meléndez J., Asplund M., Lind K., 2010, A&A, 519, A87
Chaintreuil S., Deru A., Baudin F., Ferrigno A., Grolleau E., Romagnan R., CoRot Team, 2016, The CoRoT Legacy Book: The adventure of the ultra high precision photometry from space. EDP Sciences, Les Ulis, p. 61
Chaplin W. J. et al., 2014, ApJS, 210, 1
Christensen-Dalsgaard J., 2008, Ap&SS, 316, 113
Davies G. R. et al., 2015, MNRAS, 446, 2959
do Nascimento J. D. J. et al., 2014, ApJ, 790, L23
Ferguson J. W., Alexander D. R., Allard F., Barman T., Bodnarik J. G., Hauschildt P. H., Heffner-Wong A., Tamanai A., 2005, ApJ, 623, 585
Formicola A. et al., 2004, Phys. Lett. B, 591, 61
Fulton B. J. et al., 2016, ApJ, 830, 46
Gaia Collaboration et al., 2016, A&A, 595, A1
Gaia Collaboration et al., 2018, A&A, 616, A1
Gaia Collaboration et al., 2021, A&A, 649, A6
Garciá R. A. et al., 2014, A&A, 572, A34
Grec G., Fossat E., Pomerantz M. A., 1983, Sol. Phys., 82, 55
Grevesse N., Noels A., 1993, in Prantzos N., Vangioni-Flam E., Casse M., eds, Origin and Evolution of the Elements. Cambridge University Press, Cambridge, p. 15
Handberg R., Campante T. L., 2011, A&A, 527, A56
Harvey J., 1985, in Rolfe E., Battrick B., eds, ESA Special Publication Vol. 235, Future Missions in Solar, Heliospheric & Space Plasma Physics. ESA Publications, Noordwijk, p. 199
Huber D. et al., 2011, ApJ, 743, 143
Iglesias C. A., Rogers F. J., 1996, ApJ, 464, 943
Kjeldsen H., Bedding T. R., Christensen-Dalsgaard J., 2008, ApJ, 683, L175
Koen C., Kilkenny D., van Wyk F., Marang F., 2010, MNRAS, 403, 1949
Metcalfe T. S., Creevey O. L., Christensen-Dalsgaard J., 2009, ApJ, 699, 373
Metcalfe T. S. et al., 2012, ApJ, 748, L10
Michaud G., Proffitt C. R., 1993, in Weiss W. W., Baglin A., eds, ASP Conf. Ser. Vol. 40, Inside the Stars. Astron. Soc. Pac., San Francisco, CA, p. 246
Miglio A., Montalbán J., 2005, A&A, 441, 615
Morel P., 1997, A&AS, 124, 597
Morel P., Lebreton Y., 2008, Ap&SS, 316, 61
Morel T., Rainer M., Poretti E., Barban C., Boumier P., 2013, A&A, 552, A42
Morel T., Creevey O. L., Montalbán J., Miglio A., Willett E., 2021, A&A, 646, A78
Mosser B., Appourchaux T., 2009, A&A, 508, 877
Nissen P. E., 2016, A&A, 593, A65
Nissen P. E., Silva Aguirre V., Christensen-Dalsgaard J., Collet R., Grundahl F., Slumstrup D., 2017, A&A, 608, A112
Nsamba B. et al., 2021, MNRAS, 500, 54
Oja T., 1991, A&AS, 89, 415
Ollivier M. et al., 2016, in The CoRoT Legacy Book: The adventure of the ultra high precision photometry from space. EDP Sciences, Les Ulis, p. 41