Synthetic Spectra from 3D Models of Supernovae

2002/07/03 by R. C. Thomas, E. Baron, Thomas, R. C. +3
Earth and Planetary Sciences · Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #FOS: Physical sciences #Gamma-ray bursts and supernovae #Geological and Geophysical Studies #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/0207089

4 pages, 1 figure; to appear in Stellar Atmospheric Modeling, I. Hubeny, D. Mihalas, K. Werner eds., (San Francisco : ASP)

arxiv created 2002/07/03 · openalex publication_date 2002/07/03 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

We 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.

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