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Pleione as a Variable Star
Published online by Cambridge University Press: 14 August 2015
Extract
The well-known shell star Pleione is also an interesting variable star, BU Tau. Its variability was first discovered by Calder (1937) from photoelectric observations in the 1930's. The light curve of this star from the end of the 19th century to 1954 was studied by Binnendijk (1949, 1955). Botsula and Sharov (1959) and Sharov (1961) added some old and new observations and continued the light curve up to 1959.
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- Part 1: Observations of Be Stars
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- Copyright © Reidel 1976
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