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Rapid Light Variations of the Bright Be Star ϕ Per
Published online by Cambridge University Press: 12 April 2016
Abstract
An analysis of the UBV photometric measurements obtained at Hvar Observatory and Hp HIPPARCOS photometry has been performed in order to disclose the suspected rapid periodic variations of the Be star ϕ Per. The reliability of the derived 0.5 day period is examined and the difficulties of detecting the period due to the complex character of the light variations on the longer time-scales are outlined. Possible explanations of these rapid variations are briefly discussed.
- Type
- Part 2.2. B-Type Stars
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- Copyright © Astronomical Society of the Pacific 2002