Be Stars: Rapidly Rotating Pulsators
Solar and Stellar Astrophysics
2015-06-11 v1
Abstract
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.
Cite
@article{arxiv.1210.0784,
title = {Be Stars: Rapidly Rotating Pulsators},
author = {Th. Rivinius},
journal= {arXiv preprint arXiv:1210.0784},
year = {2015}
}
Comments
Review talk given at "XX Stellar Pulsation Conference Series: Impact of new instrumentation and new insights in stellar pulsations", Granada, 5-9 September 2011, in press in AIP Conf. Ser