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Highlights of Stellar Modeling with PHOENIX

Published online by Cambridge University Press:  26 May 2016

E. Baron ,
P. H. Hauschildt ,
F. Allard ,
E. J. Lentz ,
J. Aufdenberg ,
A. Schweitzer  and
T. Barman
E. Baron
Affiliation:
Dept. of Physics and Astronomy, University of Oklahoma, 440 W. Brooks, Rm. 131, Norman, OK 73019 USA
P. H. Hauschildt
Affiliation:
Dept. of Physics & Astronomy and Center for Simulational Physics, University of Georgia, Athens, GA 30602-2451 USA
F. Allard
Affiliation:
CRAL, Ecole Normale Superieure, 46 Allee d'Italie, Lyon, 69364 France, Cedex 07
E. J. Lentz
Affiliation:
Dept. of Physics & Astronomy and Center for Simulational Physics, University of Georgia, Athens, GA 30602-2451 USA
J. Aufdenberg
Affiliation:
Harvard-Smithsonian Center for Astrophysics, Mail Stop 15, 60 Garden Street Cambridge, MA 02138 USA
A. Schweitzer
Affiliation:
Dept. of Physics & Astronomy and Center for Simulational Physics, University of Georgia, Athens, GA 30602-2451 USA
T. Barman
Affiliation:
Dept. of Physics & Astronomy and Center for Simulational Physics, University of Georgia, Athens, GA 30602-2451 USA

Abstract

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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.

Information

Type
Session A. Current Status of Modelling
Information
Symposium - International Astronomical Union , Volume 210: Modelling of Stellar Atmospheres , 2003 , pp. 19 - 32
Copyright
Copyright © Astronomical Society of the Pacific 2003 

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