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• W3100154255 abstract "Context. Photometric variability of chemically peculiar (CP) stars of the upper main sequence is closely connected to their local stellar magnetic field and their rotational period. Long term investigations, as presented here, help us to identify possible stellar cycles (as in the Sun). Furthermore, these data provide a basis for detailed surface mapping techniques." @default.
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• W3100154255 date "2010-11-26" @default.
• W3100154255 modified "2023-09-27" @default.
• W3100154255 title "A photometric long-term study of chemically peculiar stars in open clusters" @default.
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• W3100154255 doi "https://doi.org/10.1051/0004-6361/200913789" @default.
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