Highlights of Stellar Modeling with PHOENIX

Preprint

3 September 2002

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.astro-ph/0209052

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.

Keywords

EXPANDING ATMOSPHERES
BRIEFLY DESCRIBE
STELLAR MODELING
LINE BLANKETED
II SUPERNOVAE
SPHERICALLY
PHOENIX
STARS

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Version 1, 2002-09-03, ArXiv

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