Rotational velocity versus mass loss in Be stars

Details Rotational velocity versus mass loss in Be stars Rotational velocity versus mass loss in Be stars

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982iaus...98..319d&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

9

Angular Velocity, B Stars, Resonance Lines, Stellar Mass Ejection, Stellar Rotation, Spectral Line Width, Stellar Envelopes, Stellar Winds

Scientific paper

C IV and Si IV resonance line profiles of 21 Be, B-shell and normal
stars are studied with the aim of detecting evidences for mass loss. It
is found that almost all sampled here are losing mass. A relation
between an estimated lower limit for the rate of mass loss and the
observed rotational velocity was searched for but not found.

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