Synthetic Spectra from 3D Models of Supernovae

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dc.creatorThomas, R. C.
dc.creatorBaron, E.
dc.creatorBranch, David
dc.date2002-07-03
dc.date.accessioned2026-07-07T02:04:10Z
dc.date.available2026-07-07T02:04:10Z
dc.descriptionWe describe Brute, a code for generating synthetic spectra from 3D supernova models. It is based on a Monte Carlo implementation of the Sobolev approximation. The current version is highly parameterized, but in the future it will be extended for full NLTE spectrum modelling of supernovae.
dc.description4 pages, 1 figure; to appear in Stellar Atmospheric Modeling, I. Hubeny, D. Mihalas, K. Werner eds., (San Francisco : ASP)
dc.identifierhttps://arxiv.org/abs/astro-ph/0207089
dc.identifierhttp://arxiv.org/abs/astro-ph/0207089
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4648
dc.subjectAstrophysics
dc.titleSynthetic Spectra from 3D Models of Supernovae
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