Effective temperatures of CP stars

Details Effective temperatures of CP stars Effective temperatures of CP stars

1998-05-12

arxiv.org/abs/astro-ph/9805149v1

Astronomy and Astrophysics

Astrophysics

3 pages, 1 figure, to appear in: Proc. of the 26th workshop of the European Working Group on CP stars, eds. P. North, A. Schne

Scientific paper

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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