Optically Thick Winds of Hot Stars: What Determines the Mass Flux?

Details Optically Thick Winds of Hot Stars: What Determines the Mass Flux? Optically Thick Winds of Hot Stars: What Determines the Mass Flux?

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..388..207n&link_type=abstract

Mass Loss from Stars and the Evolution of Stellar Clusters ASP Conference Series, Vol. 388, proceedings of the conference held 2

Astronomy and Astrophysics

Astronomy

Scientific paper

The sonic points of optically thick winds of WNE stars are located at
large optical depth. We found that the matter flow of WNE stars starts
in very deep layers just around the convective core. This also seems to
be the case in O-star winds.

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