The B0.5IVe CoRoT target HD 49330. I. Photometric analysis from CoRoT data - Université Pierre et Marie Curie Accéder directement au contenu
Article Dans Une Revue Astronomy and Astrophysics - A&A Année : 2009

The B0.5IVe CoRoT target HD 49330. I. Photometric analysis from CoRoT data

Résumé

Context: Be stars undergo outbursts producing a circumstellar disk from the ejected material. The beating of non-radial pulsations has been put forward as a possible mechanism of ejection.
Aims: We analyze the pulsational behavior of the early B0.5IVe star HD 49330 observed during the first CoRoT long run towards the Galactical anticenter (LRA1). This Be star is located close to the lower edge of the beta Cephei instability strip in the HR diagram and showed a 0.03 mag outburst during the CoRoT observations. It is thus an ideal case for testing the aforementioned hypothesis.
Methods: We analyze the CoRoT light curve of HD 49330 using Fourier methods and non-linear least square fitting.
Results: In this star, we find pulsation modes typical of beta Cep stars (p modes) and SPB stars (g modes) with amplitude variations along the run directly correlated with the outburst. These results provide new clues about the origin of the Be phenomenon as well as strong constraints on the seismic modelling of Be stars.
Fichier principal
Vignette du fichier
aa11928-09.pdf (3.46 Mo) Télécharger le fichier
Origine : Fichiers éditeurs autorisés sur une archive ouverte

Dates et versions

hal-03785200 , version 1 (07-10-2022)

Identifiants

Citer

Anne-Laure Huat, Anne-Marie Hubert, Frederic Baudin, Michèle Floquet, Coralie Neiner, et al.. The B0.5IVe CoRoT target HD 49330. I. Photometric analysis from CoRoT data. Astronomy and Astrophysics - A&A, 2009, 506, pp.95-101. ⟨10.1051/0004-6361/200911928⟩. ⟨hal-03785200⟩
46 Consultations
5 Téléchargements

Altmetric

Partager

Gmail Facebook X LinkedIn More