M. M. Miller Bertolami, A. H. Córsico, L. G. Althaus
We present results of an ongoing study of the pulsational properties of sdB
stellar models aimed at exploring the consequences of detailed chemical
transitions for radial, $p-$ and $g-$ modes. In particular, we focus on the
effects of diffusion at the H-He transition and of He-burning at the convective
cores.
We find that diffusion of He and H has a strong impact on the period spectrum
of sdBVs stars, leading to less efficient mode trapping. Our results also
suggests that asteroseismology of sdBVs stars might offer a very good
opportunity to constrain extramixing processes in the He-burning cores of
horizontal branch stars.
View original:
http://arxiv.org/abs/1111.2335
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