Bibcode
Godart, M.; Scuflaire, R.; Thoul, A.; Noels, A.
Referencia bibliográfica
Communications in Asteroseismology, vol. 147, p. 117-120
Advertised on:
1
2006
Número de citas
0
Número de citas referidas
0
Descripción
Beta Cephei stars have a simple structure: a convective core surrounded
by a radiative envelope. It is therefore worth trying to describe beta
Cephei stars with composite polytropes which are useful to retrieve
structure parameters from frequency spectra. We show that the structure
of beta Cephei models can relatively well be described with two-zone
polytropic models. However this description is not convincing to depict
oscillations of beta Cephei models.