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Search for a Magnetic Field in the B2IV Star V 2052 Oph
Published online by Cambridge University Press: 12 April 2016
Abstract
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We have searched for magnetic signatures in the B2IV star V 2052 Oph, a β Cep star with stellar wind behavior typical for an oblique magnetic rotator, as β Cep itself. From UV spectroscopy we determined an accurate rotational period and v sin i and present the magnetic measurements as a function of rotational phase. The (small) class of magnetic pulsating early B stars are of great asteroseismological interest.
- Type
- Part 2.2. B-Type Stars
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- Copyright
- Copyright © Astronomical Society of the Pacific 2002
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