Establishing the accuracy of asteroseismic mass and radius estimates of giant stars

Autor: K. Brogaard, T. Arentoft, D. Slumstrup, F. Grundahl, M. N. Lund, L. Arndt, S. Grund, J. Rudrasingam, A. Theil, K. Christensen, M. Sejersen, F. Vorgod, L. Salmonsen, L. Ørtoft Endelt, S. Dainese, S. Frandsen, A. Miglio, J. Tayar, D. Huber

Publikováno v: Brogaard, K, Arentoft, T, Slumstrup, D, Grundahl, F, Lund, M N, Arndt, L, Grund, S, Rudrasingam, J, Theil, A, Christensen, K, Sejersen, M, Vorgod, F, Salmonsen, L, Endelt, L Ø, Dainese, S, Frandsen, S, Miglio, A, Tayar, J & Huber, D 2022, ' Establishing the accuracy of asteroseismic mass and radius estimates of giant stars : III. KIC 4054905, an eclipsing binary with two 10 Gyr thick disk RGB stars ', Astronomy and Astrophysics, vol. 668, A82 . https://doi.org/10.1051/0004-6361/202244345
Astronomy and astrophysics, Les Ulis : EDP Sciences, 2022, vol. 668, art. no. A82, p. [1-11]

Eclipsing binary stars with an oscillating giant component allow accurate stellar parameters to be derived and asteroseismic methods to be tested and calibrated. To this aim, suitable systems need to be firstly identified and secondly measured precis

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9f9a93c7853951cd84287bb517760916
https://doi.org/10.1051/0004-6361/202244345