Effective temperatures of CP stars

1998/05/12 by N. A. Sokolov, Sokolov, N. A.
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #Pulsars and Gravitational Waves Research #Solar and Space Plasma Dynamics #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/9805149

3 pages, 1 figure, to appear in: Proc. of the 26th workshop of the European Working Group on CP stars, eds. P. North, A. Schnell and J. Ziznovsky, Contrib. Astr. Obs. Skalnate Pleso Vol. 27, No 3

arxiv created 1998/05/12 · openalex publication_date 1998/05/12 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

A new method of T_eff determination for CP stars is proposed. The method is based on the fact that the slope of the energy distribution in the Balmer continuum near the Balmer jump is identical for "normal" main sequence stars and for CP stars with the same T_eff. It is shown that the T_eff of CP stars derived by this method are in good agreement with those derived by other methods.

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