NLTE Radiative Transfer and Model Atmospheres of Hot Stars

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dc.creatorWerner, K.
dc.date2002-08-15
dc.date.accessioned2026-07-07T02:04:42Z
dc.date.available2026-07-07T02:04:42Z
dc.descriptionWe 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.
dc.description12 pages, To be published in: Modelling of Stellar Atmospheres, N.E. Piskunov, W.W. Weiss, D.F. Gray, eds., Proc. IAU Symp. 210
dc.identifierhttps://arxiv.org/abs/astro-ph/0208294
dc.identifierhttp://arxiv.org/abs/astro-ph/0208294
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4856
dc.subjectAstrophysics
dc.titleNLTE Radiative Transfer and Model Atmospheres of Hot Stars
dc.typetext

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