Light variations in several broad-lined B stars

Details Light variations in several broad-lined B stars Light variations in several broad-lined B stars

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982iaus...98...49j&link_type=abstract

In: Be stars; Proceedings of the Symposium, Munich, West Germany, April 6-10, 1981. (A83-10301 01-90) Dordrecht, D. Reidel Publi

Physics

8

B Stars, Light Curve, Stellar Spectrophotometry, Variable Stars, Stellar Envelopes, Stellar Rotation

Scientific paper

Attention is given to the photometric behavior of 14 early B stars with nebulous lines, of which four appear to be pertinent to the study of Be stars. These stars are HR 2364, HR 3186, HD 72014, and HD 85860. Present results show that the variability of HR 3186 may be due to photospheric and/or shell activity, although fast rotation and large scale surface motions may also play a role. It is possible that HR 2364 and HD 85860 are variables of the same kind.

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