Time-dependent convection seismic study of delta Sct stars - Université Pierre et Marie Curie Accéder directement au contenu
Article Dans Une Revue Monthly Notices of the Royal Astronomical Society Année : 2005

Time-dependent convection seismic study of delta Sct stars

Résumé

We apply for the first time the time-dependent convection (TDC) treatment of Gabriel and Grigahcène et al. to the mode identification and seismic study of delta Sct stars. We consider the influence of this treatment on the photometric amplitude ratios and phase differences, and compare our TDC results to frozen convection (FC) results. We also compare the results obtained with different values of the mixing-length (ML) parameter alpha. Finally, we identify the modes and perform a seismic study of the stars V784 Cassiopeae (Cas), 1 Monocerotis (Mon) and 28 Andromedae (And), and show that our TDC models agree better with observations than FC models.
Fichier principal
Vignette du fichier
361-2-476.pdf (356.6 Ko) Télécharger le fichier
Origine : Fichiers éditeurs autorisés sur une archive ouverte

Dates et versions

hal-03733277 , version 1 (21-10-2022)

Identifiants

Citer

Marc-Antoine Dupret, A. Grigahcène, Rafael Garrido, Joris de Ridder, Richard Scuflaire, et al.. Time-dependent convection seismic study of delta Sct stars. Monthly Notices of the Royal Astronomical Society, 2005, 361, pp.476-486. ⟨10.1111/j.1365-2966.2005.09187.x⟩. ⟨hal-03733277⟩
20 Consultations
14 Téléchargements

Altmetric

Partager

Gmail Facebook X LinkedIn More