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NLTE Radiative Transfer and Model Atmospheres of Hot Stars
Published online by Cambridge University Press: 26 May 2016
Abstract
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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
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