CAOSP abstracts, Volume: 27, No.: 3, year: 1998
- Author(s): SOKOLOV, N.A.
- Journal: Contributions of the Astronomical Observatory Skalnate Pleso,
vol. 27, no. 3, p. 261-263.
- Date: 04/1998
- Title: Effective temperatures of CP stars
- Keyword(s): CHEMICALLY PECULIAR STARS, FUNDAMENTAL PARAMETERS
- Pages: 261 -- 263
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.
Full text version of this article in
(600dpi) format compressed by gzip; or in