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Autor:
Mikulášek, Zdeněk, Krtička, Jiří, Janík, Jan, Zejda, Miloslav, Henry, Gegory W., Paunzen, Ernst, Žižňovský, Jozef, Zverko, Juraj
The majority of magnetic chemically peculiar (mCP) stars exhibit periodic light, magnetic, radio, and spectroscopic variations that can be adequately modelled as a rigidly-rotating main-sequence star with persistent surface structures. Nevertheless,
Externí odkaz:
http://arxiv.org/abs/1310.6640