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Pleione as a Variable Star

Published online by Cambridge University Press:  14 August 2015

A. S. Sharov  and
V. M. Lyuty
A. S. Sharov
Affiliation:
Moscow University, Moscow, U.S.S.R.
V. M. Lyuty
Affiliation:
Moscow University, Moscow, U.S.S.R.

Extract

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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.

Type
Part 1: Observations of Be Stars
Information
Symposium - International Astronomical Union , Volume 70: Be and Shell Stars , 1976 , pp. 105 - 106
Copyright
Copyright © Reidel 1976 

References

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