[en] In this paper, we give an updated overview of the observed characteristics of g-mode pulsations in slowly pulsating B stars. These characteristics are based on the combined results of linear nonadiabatic analysis of the oscillations and a photometric and spectroscopic mode identification for a sample of 13 members. For 4 stars, at least one mode is stable in all the considered theoretical models.
Dupret, Marc-Antoine ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique
Scuflaire, Richard ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Evol. et stabilité des étoiles et des amas d'étoiles (ESEA)
De Ridder, J.
Niemczura, E.
Aerts, C.
Language :
English
Title :
g-mode pulsations in slowly pulsating B stars
Publication date :
01 May 2004
By request :
Yes
Audience :
International
Main work title :
IAU Colloq. 193: Variable Stars in the Local Group