Effect of mass loss on the driving of g-modes in B supergiant stars

Bibcode
2008JPhCS.118a2055G
DOI
10.1088/1742-6596/118/1/012055
Godart, Mélanie; Noels, Arlette; Dupret, Marc-Antoine
Referencia bibliográfica

Journal of Physics: Conference Series, Volume 118, Issue 1, id. 012055 (2008).

Fecha de publicación:
10
2008
Número de autores
3
Número de autores del IAC
0
Número de citas
1
Número de citas referidas
0
Descripción
MOST has detected p and g-modes in the B supergiant star HD163899. Saio et al. (2006) have explained the driving of g-modes in a post main sequence star by the presence of a convective shell which prevents some modes from entering the damping radiative core. We show that this scenario depends on the evolution of the star, with or without mass loss. If the mass loss rate is high enough, the convective shell disappears and all the g-modes are stable.
Tipo
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