Hostname: page-component-cd9895bd7-dk4vv Total loading time: 0 Render date: 2024-12-26T05:33:04.108Z Has data issue: false hasContentIssue false

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

Published online by Cambridge University Press:  12 April 2016

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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
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, 387403.Google Scholar
Straizys, V., Kuriliene, G., 1981. Astr. Sp. Sci., 80, 353368.CrossRefGoogle Scholar
1977.