Article contents
NLTE Radiative Transfer and Model Atmospheres of Hot Stars
Published online by Cambridge University Press: 26 May 2016
Abstract
We describe our method to construct line blanketed NLTE model atmospheres for hot stars. We employ the Accelerated Lambda Iteration and use statistical methods to deal with metal line blanketing.
- Type
- Session B. Radiative Transfer
- Information
- Symposium - International Astronomical Union , Volume 210: Modelling of Stellar Atmospheres , 2003 , pp. 81 - 92
- Copyright
- Copyright © Astronomical Society of the Pacific 2003
References
- 1
- Cited by