Atmosphere Models for Very Low Mass Stars, Brown Dwarfs and Exoplanets
Astrophysics
2009-09-25 v1
Abstract
Over the past decade considerable effort, both observational and theoretical, has been directed towards a more accurate determination of the stellar lower main sequence and of the sub-stellar domain covered by Brown Dwarfs and Planets. A review of the recent improvement in the theory of cool model atmospheres is presented.
Cite
@article{arxiv.astro-ph/9705077,
title = {Atmosphere Models for Very Low Mass Stars, Brown Dwarfs and Exoplanets},
author = {Isabelle Baraffe and France Allard},
journal= {arXiv preprint arXiv:astro-ph/9705077},
year = {2009}
}
Comments
7 pages, Latex file, uses crckapb.sty, Proc. of IAU Symp 189, "Fundamental Stellar Properties...", eds T.R Bedding, A.J Booth and J. Davis, Kluwer