Digitale Medien
Springer
Astrophysics and space science
224 (1995), S. 541-542
ISSN:
1572-946X
Schlagwort(e):
Be stars
;
wind
;
mass loss
Quelle:
Springer Online Journal Archives 1860-2000
Thema:
Physik
Notizen:
Abstract 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.
Materialart:
Digitale Medien
URL:
http://dx.doi.org/10.1007/BF00667945
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