Premium
Theoretical modelling of optical and IR spectra of brown dwarfs and ultracool dwarfs
Author(s) -
Pavlenko Y. V.
Publication year - 2005
Publication title -
astronomische nachrichten
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.394
H-Index - 63
eISSN - 1521-3994
pISSN - 0004-6337
DOI - 10.1002/asna.200510458
Subject(s) - brown dwarf , physics , spectral line , stellar classification , astrophysics , optical spectra , interpretation (philosophy) , astronomy , stars , computer science , programming language
The current state of theoretical modelling of the spectra of cool dwarfs and ultracool objects are discussed. Fits of synthetical spectral energy distributions (SEDs) in the optical and IR spectral regions to observed spectra show problems of theoretical modelling. Problems of interpretation of observed spectra are more obvious for the case of L and T dwarfs. Still even for late‐M dwarfs the situation is far from being perfect. Some examples of the .ne analysis of the spectra of ultracool dwarfs are presented. (© 2005 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)