Be Stars: Rapidly Rotating Pulsators
classification
🌌 astro-ph.SR
keywords
starsrapidlyrotatingcasesclasscontributiondipolarexception
read the original 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.
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