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.
CITATION STYLE
Rivinius, T. (2013). Be stars: Rapidly rotating pulsators. In Astrophysics and Space Science Proceedings (Vol. 31, pp. 253–259). Springer Netherlands. https://doi.org/10.1007/978-3-642-29630-7_46
Mendeley helps you to discover research relevant for your work.