NLTE Radiative Transfer and Model Atmospheres of Hot Stars
Abstract
Description
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.
12 pages, To be published in: Modelling of Stellar Atmospheres, N.E. Piskunov, W.W. Weiss, D.F. Gray, eds., Proc. IAU Symp. 210
12 pages, To be published in: Modelling of Stellar Atmospheres, N.E. Piskunov, W.W. Weiss, D.F. Gray, eds., Proc. IAU Symp. 210