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Absolute Magnitudes and Intrinsic Colours of Non-Supergiant Be Stars

Published online by Cambridge University Press:  14 August 2015

J. R. Kozok
J. R. Kozok*
Affiliation:
Astronomisches Institut, Ruhr-Universität, 4630 Bochum 1, FRG

Abstract

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101 normal Be stars, probable members of 56 galactic clusters and OB-associations, and more than 20 extreme Be stars in the Large Magellanic Cloud were used to derive intrinsic colours of 09-B9 (III-V)e stars. Furthermore, the correlation between the intrinsic colour (U-B)0 and the absolute magnitude of non-supergiant Be stars was confirmed to be and

The aim of the present investigation is to enlarge the basis for the determination of intrinsic colours and absolute magnitudes by providing a large sample from the southern sky.

Type
I. Photometry
Information
Symposium - International Astronomical Union , Volume 98: Be Stars , 1982 , pp. 33 - 36
Copyright
Copyright © Reidel 1982 

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