Early Spectra of Supernovae
Astrophysics
2007-05-23 v1
Abstract
We 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.
Cite
@article{arxiv.astro-ph/0409659,
title = {Early Spectra of Supernovae},
author = {E. Baron and Peter Nugent and David Branch and Peter H. Hauschildt},
journal= {arXiv preprint arXiv:astro-ph/0409659},
year = {2007}
}
Comments
To appear in 1604-2004 Supernovae As Cosmological Lighthouses, (San Francisco: ASP), 6 pages