NLTE Radiative Transfer and Model Atmospheres of Hot Stars

2002/08/15 by K. Werner, Werner, K.
Mathematics · Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #FOS: Physical sciences #Scientific Research and Discoveries #Statistical and numerical algorithms #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/0208294

12 pages, To be published in: Modelling of Stellar Atmospheres, N.E. Piskunov, W.W. Weiss, D.F. Gray, eds., Proc. IAU Symp. 210

arxiv created 2002/08/15 · openalex publication_date 2002/08/15 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

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.

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