Effective temperatures of Ap stars (Sokolov, 1998)

Details Effective temperatures of Ap stars (Sokolov, 1998) Effective temperatures of Ap stars (Sokolov, 1998)

Jul 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ycat..41300215s&link_type=abstract

VizieR On-line Data Catalog: J/A+AS/130/215. Originally published in: 1998A&AS..130..215S

Physics

Stars: Peculiar, Effective Temperatures

Scientific paper

A new method of determination of the effective temperatures of Ap stars is proposed. The method is based on the fact that the slopes of the energy distribution in the Balmer continuum near the Balmer jump for "normal" main sequence stars and Ap stars with the same effective temperature are identical. The effective temperature calibration is based on a sample of main sequence stars with well known temperatures (Sokolov, 1995, Cat. ).
(1 data file).

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