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Investigations of the Magnetic Fields of Chemically Peculiar Stars of Different Age

Published online by Cambridge University Press:  12 April 2016

Yu.V. Glagolevskij ,
V.G. Klochkova  and
I.M. Kopylov
Yu.V. Glagolevskij
Affiliation:
Special Astrophysical Observatory of USSR Academy of Sciences, Nizhnij Arkhyz
V.G. Klochkova
Affiliation:
Special Astrophysical Observatory of USSR Academy of Sciences, Nizhnij Arkhyz
I.M. Kopylov
Affiliation:
Special Astrophysical Observatory of USSR Academy of Sciences, Nizhnij Arkhyz

Abstract

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The program of comprehensive investigations of stellar magnetism in the Special Astrophysical Observatory of the USSR AS includes the study of origin and evolution of the stellar magnetic fields in open clusters and associations of different age. In the papers by Borra (1981), Brown et al. (1981) and North and Cramer (1984) have been found some indications on the evolutionary decay of the fossil stellar fields.

Type
Section I - Theoretical Considerations
Information
International Astronomical Union Colloquium , Volume 90: Upper Main Sequence Stars with Anomalous Abundances , 1986 , pp. 29 - 32
Copyright
Copyright © Reidel 1986

References

Borra, E., 1981. Astrophys. J., Letters, 249, L39 – L42.CrossRefGoogle Scholar
Brown, D.N., Landstreet, J.D., Thompson, I., 1981. 23-d Liege Coll, p. 195 – 198.Google Scholar
North, P., Cramer, N., 1984. Astron. Astrophys., Suppl. Ser., 58, 387–403.Google Scholar
Straizys, V., Kuriliene, G., 1981. Astr. Sp. Sci., 80, 353–368.CrossRefGoogle Scholar
1977.