Rotation, expansion and duplicity of Be stars

Details Rotation, expansion and duplicity of Be stars Rotation, expansion and duplicity of Be stars

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982iaus...98..279h&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

Computer Science

23

B Stars, Binary Stars, Stellar Mass Ejection, Stellar Models, Stellar Rotation, Statistical Analysis, Stellar Envelopes, Stellar Luminosity, Stellar Spectra

Scientific paper

The three general concepts proposed as explanations for the Be star phenomenon in all its complexity are considered. These include the rotational hypothesis of Struve (1931), the radial outflow of matter hypothesized by Gerasimovic (1934), and the binary hypothesis formulated by Kriz and Harmanec (1975). An attempt is made to identify the attractive features and the pitfalls of these three positions in light of recent observational data.

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