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On the Magnetic Field of β CrB
Published online by Cambridge University Press: 12 April 2016
Abstract
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We have discussed the oscillations of the magnetic field (He) of β CrB with a period P2=P1/5=3d.6974, where P1 is stimulated by a rotation of the star. The analysis of other author’s measurements has been confirmed the reality of P2.
- Type
- Section I - Theoretical Considerations
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- Copyright
- Copyright © Reidel 1986
References
Plachinda, S.I. Izv. Krimsk. Astrofiz. Obs., 74, (in press).Google Scholar
Preston, G.W., and Sturch, C.
1967, in The Magnetic and Related Stars, ed. Cameron, R.C. (Baltimore: Mono Book Corp.), p. 111.Google Scholar
Severny, A.B., Kuvshinov, V.M., and Nikulin, N.S.
1974, Izv. Krimsk. Astrofiz. Obs., 50, 3.Google Scholar
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