The geometry of decoupled line driven winds

Details The geometry of decoupled line driven winds The geometry of decoupled line driven winds

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.224..541p&link_type=abstract

Astrophysics and Space Science, Volume 224, Issue 1-2, pp. 541-542

Astronomy and Astrophysics

Astrophysics

Be Stars, Wind, Mass Loss

Scientific paper

Bjorkman & Cassinelli (1993) have proposed a mechanism that is expected to produce strong equatorial focusing of the radiation-driven winds from rapidly-rotating B stars. Here the possibility of the decoupling of the stellar radiation field and the outflow is considered. We find that greater equator to pole density ratios may be generated than the standard model, bringing it more into line with results implied by observations.

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