2005/06/13 by Ya. V. Pavlenko, Yakiv V. Pavlenko, Pavlenko, Yakiv V.
Physics and Astronomy · #Astro and Planetary Science #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #FOS: Physical sciences #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0506263
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
arxiv created 2005/06/13 · openalex publication_date 2005/06/13 · arxiv updated 2009/12/01 · openalex created_date 2024/04/10 · openalex updated_date 2026/07/28
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.