On the Magnetic Field of β CrB

Plachinda, S. I.

doi:10.1007/978-94-009-4714-6_7

S. I. Plachinda⁴

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 125))

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Abstract

We have discussed the oscillations of the magnetic field (H_e) of β CrB with a period P₂=P₁/5= =3^d.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.

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Authors and Affiliations

Crimean Astrophysical Observatory, Nauchny Crimea, SU - 334413, USSR
S. I. Plachinda

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S. I. Plachinda
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Department of Astronomy, The University of Michigan, Ann Arbor, Michigan, USA
C. R. Cowley
Department of Physics and Astronomy, University College London, UK
M. M. Dworetsky
Observatoire de Paris, Meudon, France
C. Mégessier

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Plachinda, S.I. (1986). On the Magnetic Field of β CrB. In: Cowley, C.R., Dworetsky, M.M., Mégessier, C. (eds) Upper Main Sequence Stars with Anomalous Abundances. Astrophysics and Space Science Library, vol 125. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-4714-6_7

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DOI: https://doi.org/10.1007/978-94-009-4714-6_7
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-8597-7
Online ISBN: 978-94-009-4714-6
eBook Packages: Springer Book Archive

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