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- W3104734887 abstract "Context. The (magnetic) chemically peculiar (CP) stars of the upper main sequence are well-suited laboratories for investigating the influence of magnetic fields on the stellar surface because they produce abundance inhomogeneities (spots), which results in photometric variability that is explained in terms of the oblique rotator model. CP stars exhibiting this phenomenon are normally classified as α2 Canum Venaticorum (ACV) variables. It is important to increase the sample of known rotational periods among CP stars by discovering new ACV variables. An increased sample size will contribute to the understanding of the CP stars’ evolution in time." @default.
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- W3104734887 date "2015-09-01" @default.
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- W3104734887 title "A search for photometric variability in magnetic chemically peculiar stars using ASAS-3 data" @default.
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- W3104734887 doi "https://doi.org/10.1051/0004-6361/201526424" @default.
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