Journal Article

The magnetic field and rotational period of 53 Camelopardalis

G. M. Hill, D. A. Bohlender, J. D. Landstreet, G. A. Wade, N. Manset and P. Bastien

in Monthly Notices of the Royal Astronomical Society

Published on behalf of The Royal Astronomical Society

Volume 297, issue 1, pages 236-238
Published in print June 1998 | ISSN: 0035-8711
Published online June 1998 | e-ISSN: 1365-2966 | DOI: http://dx.doi.org/10.1046/j.1365-8711.1998.01473.x
The magnetic field and rotational period of 53 Camelopardalis

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The magnetic Ap star 53 Cam has been described as the best object for testing theories of elemental diffusion in the presence of a stellar magnetic field. It is thus vital to determine the rotational period of this very important star as accurately as possible. An improved period (8.026 81±0.000 04 d) is derived here by combining new measurements of the effective magnetic field with previously published values.

Keywords: stars: chemically peculiar; stars: individual: HD 65339; stars: magnetic fields

Journal Article.  0 words. 

Subjects: Astronomy and Astrophysics

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