Back to Volume
Paper: Optically Thick Winds of Hot Stars: What Determines the Mass Flux?
Volume: 388, Mass Loss from Stars and the Evolution of Stellar Clusters
Page: 207
Authors: Nugis, T.
Abstract: 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.
Back to Volume