Highlights of Stellar Modeling with PHOENIX

Details Highlights of Stellar Modeling with PHOENIX Highlights of Stellar Modeling with PHOENIX

2002-09-03

arxiv.org/abs/astro-ph/0209052v1

Astronomy and Astrophysics

Astrophysics

12 pages, 7 figures, to appear in Modeling of Stellar Atmospheres, IAU Symposium 210, Nikolai Piskunov David Gray, and Werner

Scientific paper

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.

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