Please use this identifier to cite or link to this item: https://repositorio.ufrn.br/jspui/handle/123456789/28887
Title: Fundamental parameters of Be stars located in the seismology fields of COROT
Authors: Frémat, Y.
Neiner, C.
Floquet, M.
Zorec, J.
Janot-Pacheco, E.
Medeiros, José Renan de
Keywords: Stars: emission-line, Be;Stars: activity;Stars: fundamental parameters
Issue Date: 4-May-2006
Publisher: Astronomy & Astrophysics
Citation: MEDEIROS, José Renan et al. Fundamental parameters of Be stars located in the seismology fields of Corot. Astronomy & Astrophysics (Berlin), França, v. 451, n. 3, p. 1053-1063, 2006. ISSN 1432-0746. DOI https://doi.org/10.1051/0004-6361:20053305. Disponível em: https://www.aanda.org/articles/aa/abs/2006/21/aa3305-05/aa3305-05.html. Acesso em: 5 maio 2020.
Portuguese Abstract: In preparation for the COROT space mission, we determined the fundamental parameters (spectral type, temperature, gravity, Vsini) of the Be stars observable by COROT in its seismology fields (64 Be stars). We applied a careful and detailed modeling of the stellar spectra, taking into account the veiling caused by the envelope, as well as the gravitational darkening and stellar flattening due to rapid rotation. Evolutionary tracks for fast rotators were used to derive stellar masses and ages. The derived parameters will be used to select Be stars as secondary targets (i.e. observed for 5 consecutive months) and short-run targets of the COROT mission. Furthermore, we note that the main part of our stellar sample is falling in the second half of the main sequence life time, and that in most cases the luminosity class of Be stars is inaccurate in characterizing their evolutionary status.
URI: https://repositorio.ufrn.br/jspui/handle/123456789/28887
ISSN: 0004-6361 (print), 1432-0746 (online)
Appears in Collections:CCET - DFTE - Artigos publicados em periódicos

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