Chemically peculiar stars and their temperature calibration
Aims. The determination of effective temperature for chemically peculiar (CP) stars by means of photometry is a sophisticated task due to their abnormal colours. Standard calibrations for normal stars lead to erroneous results and, in most cases corrections are necessary.
Keywords: stars: chemically peculiar ; stars: fundamental parameters ; techniques: photometric ; methods: statistical ; Elemental Abundance Analyses ; Infrared Flux Method ; Helium-Weak Star ; B-Type Stars ; Optical-Region Fluxes ; Upper Main-Sequence ; Magnetic Cp-Stars ; Ap-Stars ; Dao Spectrograms ; Roap Stars
Record created on 2010-11-30, modified on 2016-08-09