Highlights of Stellar Modeling with PHOENIX
Astrophysics
2007-05-23 v1
Abstract
We briefly describe the current version of the PHOENIX code. We then present some illustrative results from the modeling of Type Ia and Type II supernovae, hot stars, and irradiated giant planets. Good fits to observations can be obtained, when account is taken for spherically symmetric, line-blanketed, static or expanding atmospheres.
Cite
@article{arxiv.astro-ph/0209052,
title = {Highlights of Stellar Modeling with PHOENIX},
author = {E. Baron and Peter H. Hauschildt and F. Allard and Eric J. Lentz and J. Aufdenberg and A. Schweitzer and T. Barman},
journal= {arXiv preprint arXiv:astro-ph/0209052},
year = {2007}
}
Comments
12 pages, 7 figures, to appear in Modeling of Stellar Atmospheres, IAU Symposium 210, Nikolai Piskunov David Gray, and Werner Weiss, eds. (San Francisco: PASP)