Physics
Scientific paper
Mar 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..361..479o&link_type=abstract
Active OB-Stars: Laboratories for Stellar and Circumstellar Physics, ASP Conference Series, Vol. 361, Proceedings of the confere
Physics
Scientific paper
While Wolf-Rayet mass-loss rates have been well-modeled using detailed radiative transfer simulations, some conceptual uncertainties still remain, such as the maximum attainable driving efficiency. To complement detailed, but conceptually complex simulations we isolate specific wind properties to derive simple analytic models and study the effect frequency redistribution has on the mass-loss rate.
Gayley Ken G.
Onifer Andrew J.
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