Highlights of Stellar Modeling with PHOENIX

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dc.creatorBaron, E.
dc.creatorHauschildt, Peter H.
dc.creatorAllard, F.
dc.creatorLentz, Eric J.
dc.creatorAufdenberg, J.
dc.creatorSchweitzer, A.
dc.creatorBarman, T.
dc.date2002-09-03
dc.date.accessioned2026-07-07T02:04:57Z
dc.date.available2026-07-07T02:04:57Z
dc.descriptionWe 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.
dc.description12 pages, 7 figures, to appear in Modeling of Stellar Atmospheres, IAU Symposium 210, Nikolai Piskunov David Gray, and Werner Weiss, eds. (San Francisco: PASP)
dc.identifierhttps://arxiv.org/abs/astro-ph/0209052
dc.identifierhttp://arxiv.org/abs/astro-ph/0209052
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4962
dc.subjectAstrophysics
dc.titleHighlights of Stellar Modeling with PHOENIX
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