Multicomponent stellar winds of B stars

Details Multicomponent stellar winds of B stars Multicomponent stellar winds of B stars

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008coska..38..425k&link_type=abstract

Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 38, no. 2, p. 425-426.

Astronomy and Astrophysics

Astronomy

Stars: Winds, Outflows, Stars: Early-Type, Hydrodynamics

Scientific paper

We study multicomponent effects in the stellar winds of B type stars.
For stars with highest mass-loss rates the usual one-component approach
is sufficient. For stars with weaker winds multicomponent effects become
important. For even less dense winds hydrogen and helium fall back on
the stellar surface or even a pure metallic wind is possible.

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