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• W33136635 endingPage "A82" @default.
• W33136635 startingPage "A82" @default.
• W33136635 abstract "Context. Chemically peculiar stars of the upper part of the main sequence show periodical variability in line intensities and continua, modulated by the stellar rotation, which is attributed to the existence of chemical spots on the surface of these stars. The flux variability is caused by the changing redistribution rate of the radiative flux predominantly from the short-wavelength part of the spectra to the long-wavelength part, which is a result of abundance anomalies. Many details of this process are still unknown." @default.
• W33136635 created "2016-06-24" @default.
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• W33136635 date "2015-04-01" @default.
• W33136635 modified "2023-10-01" @default.
• W33136635 title "Visual and ultraviolet flux variability of the bright CP star<i>θ</i>Aurigae" @default.
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• W33136635 doi "https://doi.org/10.1051/0004-6361/201425097" @default.
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