Article contents
Highlights of Stellar Modeling with PHOENIX
Published online by Cambridge University Press: 26 May 2016
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.
- 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
References
- 2
- Cited by