NLTE analysis of spectra: OBA stars
Solar and Stellar Astrophysics
2016-07-27 v1
Abstract
Methods of calculation of NLTE model atmosphere are discussed. The NLTE trace element procedure is compared with the full NLTE model atmosphere calculation. Differences between LTE and NLTE atmosphere modeling are evaluated. The ways of model atom construction are discussed. Finally, modelling of expanding atmospheres of hot stars with winds is briefly reviewed.
Keywords
Cite
@article{arxiv.1406.3556,
title = {NLTE analysis of spectra: OBA stars},
author = {Jiří Kubát and Brankica Šurlan},
journal= {arXiv preprint arXiv:1406.3556},
year = {2016}
}
Comments
in Determination of Atmospheric Parameters of B-, A-, F- and G-Type Stars, E. Niemczura et al. eds., Springer, in press