Ultracool dwarfs
Astrophysics
2007-05-23 v1
Abstract
We present results of modeling of spectra of M-, L-, T-dwarfs. Theoretical spectra are fitted to observed spectra to study the main parameters of the low-mass objects beyond the bottom of Main Sequence. Application of ``lithium'' and ``deuterium'' tests for assessment of ultra-cool dwarfs are discussed.
Keywords
Cite
@article{arxiv.astro-ph/0506263,
title = {Ultracool dwarfs},
author = {Yakiv V. Pavlenko},
journal= {arXiv preprint arXiv:astro-ph/0506263},
year = {2007}
}
Comments
Talk for MAO2004 Meeting (Kyiv, July 15-17, 2004), see more details on http://www.mao.kiev.ua/mao-2004/public.htm, 6 pages, 3figs