Ledoux's convection criterion in evolution and asteroseismology of massive stars
Saio et al. (2006) have shown that the presence of an intermediate convective zone (ICZ) in post-main sequence models could prevent the propagation of g-modes in the radiative interior and hence avoid the corresponding radiative damping. The development of such a convective region highly depends on the structure of the star in the μ-gradient region
Lebreton, Y. et al.
Advertised on:
7
2009