Early Spectra of Supernovae

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dc.creatorBaron, E.
dc.creatorNugent, Peter
dc.creatorBranch, David
dc.creatorHauschildt, Peter H.
dc.date2004-09-27
dc.date.accessioned2026-07-07T02:14:46Z
dc.date.available2026-07-07T02:14:46Z
dc.descriptionWe briefly describe the current version of the PHOENIX code. We then present some results on the modeling of Type II supernovae and show that fits to observations can be obtained, when account is taken for spherically symmetric, line-blanketed, expanding atmospheres. We describe the SEAM method of obtaining distances to supernovae and briefly discuss its future prospects.
dc.descriptionTo appear in 1604-2004 Supernovae As Cosmological Lighthouses, (San Francisco: ASP), 6 pages
dc.identifierhttps://arxiv.org/abs/astro-ph/0409659
dc.identifierhttp://arxiv.org/abs/astro-ph/0409659
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8250
dc.subjectAstrophysics
dc.titleEarly Spectra of Supernovae
dc.typetext

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