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BCD Spectrophotometry of the Be-Shell Star 88 Her

Published online by Cambridge University Press:  14 August 2015

L. Divan  and
J. Zorec
L. Divan
Affiliation:
Institut d'Astrophysique de Paris, France
J. Zorec
Affiliation:
Laboratoire d'Astrophysique Théorique, Collège de France

Extract

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The spectrophotometric behavior of the Be/shell stars seems to be different when their second Balmer discontinuity is in emission from that when it is in absorption. We have analysed here a particular case in which the second Balmer jump is in absorption. In this note we compare the results of a BCD analysis concerning the variations of the Be-Shell star 88 Her (HD162732), to the results of the UBV photometry.

Type
I. Photometry
Information
Symposium - International Astronomical Union , Volume 98: Be Stars , 1982 , pp. 61 - 63
Copyright
Copyright © Reidel 1982 

References

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