WR Wind Models: [WC]-Type CSPN vs. Massive Stars

Details WR Wind Models: [WC]-Type CSPN vs. Massive Stars WR Wind Models: [WC]-Type CSPN vs. Massive Stars

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..391...99g&link_type=abstract

Hydrogen-Deficient Stars ASP Conference Series, Vol. 391, proceedings of the conference held 17-21 September, 2007, at Eberhard

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Scientific paper

The optically thick stellar winds of Wolf-Rayet (WR) stars have recently been explained by means of hydrodynamic model atmospheres. In the present talk we discuss the physical processes that lead to their formation for the case of young massive stars as well as for [WC]-type CSPN. We explain why we expect WR-type mass loss only in specific temperature regimes, and discuss the possibility of pulsational wind driving for other cases.

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