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Some Photometric Characteristics of be Stars (Review Paper)

Published online by Cambridge University Press:  14 August 2015

E. Eugenio  and
V. Mendoza
E. Eugenio
Affiliation:
Instituto de Astronomía, Universidad Nacional Autónoma de México
V. Mendoza
Affiliation:
Instituto de Astronomía, Universidad Nacional Autónoma de México

Abstract

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Homogeneous observational data on four photometric systems which cover the spectral range from 0.14 to 4 microns through narrow, intermediate and broad passband filters are used to review and derive some photometric characteristics of Be stars. We find that 60% of the stars under discussion have ultraviolet and infrared excesses.

Type
I. Photometry
Information
Symposium - International Astronomical Union , Volume 98: Be Stars , 1982 , pp. 3 - 17
Copyright
Copyright © Reidel 1982 

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