No CrossRef data available.
Article contents
Wind Models for O-type Stars
Published online by Cambridge University Press: 26 May 2016
Abstract
We present fully consistent models for O-type stars that reproduce the observed UV spectra simultaneously with the observed terminal velocities and mass loss rates. We demonstrate how, as a consequence, the models can be used to determine the stellar parameters from the observed UV spectra alone.
- Type
- Part IV: Central Stars and their Atmospheres
- Information
- Copyright
- Copyright © Astronomical Society of the Pacific 2003