对称星体中热成分的星际大气与吸积盘模型
天体物理学
2007-05-23 v1
摘要
我们描述了用于计算热星体和吸积盘合成光谱的 NLTE 代码。这两种代码可组合用于计算对称星体中热成分的致动子通量。
引用
@article{arxiv.astro-ph/0208199,
title = {Stellar Atmosphere and Accretion Disk Models for the Hot Component in Symbiotic Stars},
author = {K. Werner and J. L. Deetjen and S. Dreizler and T. Nagel and T. Rauch},
journal= {arXiv preprint arXiv:astro-ph/0208199},
year = {2007}
}
备注
To be published in: Symbiotic stars probing stellar evolution, R.L.M. Corradi, J. Mikolajewska, and T.J. Mahoney, eds., ASP Conference Series, 4 pages, no figures