부산대학교 도서관

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.
Comment: 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)