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Cycle to Cycle Irregularities in the Monoperiodic β Cephei Star BW Vulpeculae
Published online by Cambridge University Press: 12 April 2016
Abstract
High spectral and time resolution observations show that the monoperiodic β Cephei star BW Vul presents differences in both line profiles and velocities from one cycle to another, which may be due to the consequence of the passage of two strong shock waves.
- Type
- Part 2.2. B-Type Stars
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- Copyright © Astronomical Society of the Pacific 2002