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Cool Magnetic CP Stars
Published online by Cambridge University Press: 12 April 2016
Abstract
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We review progress in research on the cool magnetic CP stars especially during the past four years. Studies of energy distributions and abundances are analyzed to reveal their systematics. Model atmospheres do not yet accurately describe the average energy distributions much less the variability with the rotational periods of these stars.
- Type
- Section III - Magnetic CP Stars
- Information
- Copyright
- Copyright © Reidel 1986
References
Biemont, E., Karner, C., Meyer, G., Trager, F., zu Putlitz, G.: 1982, Astron. Astrophys.
107, 166
Google Scholar
Hardorp, J., Shore, S.N., Witmann, A.: 1976, Physics of Ap-Stars, Weiss, W.W., Jenkner, H., Wood, H.J., eds., University of Vienna Observatory, p. 419
Google Scholar
Piskunov, N.E., Khokhlova, V.L.: 1984, 6th Sci. Conf. Subcommission 4 Multilateral Cooperation Acad. Sci. Socialist Countries, 20Google Scholar
Ryabchikova, T.A., Piskunov, N.E.: 1984, 6th Sci.Conf. Subcommision 4 Multilateral Cooperation Acad. Sci. Socialist Countries, 27Google Scholar
Ryabchikova, T.A., Ptitsyn, D.A.: 1986, Upper Main Sequence Stars With Anomalous Abundances, Cowley, C.R., Megessier, C., eds. (this conference)Google Scholar
Van Dijk, W., Kerssies, A., Hammerschlag-Hensberge, G., Wesslies, P.R.: 1978, Astron. Astrophys. Suppl.
66, 187
Google Scholar
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