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Differential Rotation in B and Be Stars
Published online by Cambridge University Press: 23 September 2016
Summary
In this paper we present two kinds of results which show that differential rotation is a highly probable phenomenon in B and Be stars. These results show that angular momentum is an important parameter which must be taken into account for interpreting the observed parameters of B and Be stars and for studying their structure.
- Type
- IIA. The Underlying Stars: Observations
- Information
- International Astronomical Union Colloquium , Volume 92: Physics of Be Stars , August 1987 , pp. 68 - 71
- Copyright
- Copyright © Cambridge University Press 1987
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