2002/09/02 by Ya. V. Pavlenko, Yakiv V. Pavlenko, Pavlenko, Yakiv V.
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #FOS: Physical sciences #Scientific Research and Discoveries #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0209022
9 pages, 12 figs, summitted to Proc. of IAU110, Uppsala
arxiv created 2002/09/02 · openalex publication_date 2002/09/02 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Procedure and results of computations of stellar model atmospheres and spectral energy distributions are discussed. Model atmospheres of some chemically peculiar stars are computed taking into account detailed information about their abundances: -- R CrB-like stars of Teff ∼ 7000 K, -- Sakurai's object (V4334 Sgr) of 4000