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Model atmosphere parameters of the binary systems COU1289 and COU1291
Author(s) -
AlWardat M. A.
Publication year - 2007
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.200510676
Subject(s) - physics , atmosphere (unit) , astrophysics , binary number , spectral line , spectral energy distribution , binary system , energy (signal processing) , stellar atmosphere , observatory , thermodynamics , stars , astronomy , mathematics , arithmetic , quantum mechanics , galaxy
Abstract The spectral energy distributions between λ 3700 Å and λ 8100 Å of the binary systems COU1289 and COU1291 have been measured with the Carl‐Zeiss‐Jena 1 m telescope of the Special Astrophysical Observatory. Their B, V, R magnitudes and B – V colour indices were computed and compared with earlier investigations. Model atmospheres of both systems were constructed using a grid of Kurucz blanketed models, their spectral energy distributions in the continuous spectrum were computed and compared with the observational ones. The model atmosphere parameters for the components of COU1289 were derived as: T a eff = 7100 K, T b eff = 6300 K, log g a = 4.22, log g b = 4.22, R a = 1.50 R ⊙ , R b = 1.40 R ⊙ , and for the components of COU1291 as: T a eff = 6400 K, T b eff = 6100 K, log g a = 4.20, log g b = 4.35, R a = 1.47 R ⊙ , R b = 1.12 R ⊙ . The spectral types of both components of the system COU1289 were concluded as F1 and F7, and of the system COU1291 as F6 and F9. Finally the formation and evolution of the systems were discussed. (© 2007 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)