1210.0784 (Th. Rivinius)

Be Stars: Rapidly Rotating Pulsators    [PDF]

Th. Rivinius

I will show that Be stars are, without exception, a class of rapidly rotating stars, which are in the majority of cases pulsating stars as well, while none of them does possess a large scale (i.e. with significant dipolar contribution) magnetic field.

View original: http://arxiv.org/abs/1210.0784