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Are Classical Be Stars Sources of Hard X-Rays?

Published online by Cambridge University Press:  14 August 2015

Geraldine J. Peters
Geraldine J. Peters*
Affiliation:
Department of Astronomy, University of Southern California, Los Angeles, CA 90007 USA

Abstract

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A point summation technique was used to search the UHURU data base for X-ray emission from classical Be stars. Of the thirty-two stars considered, only three (λ Cas, HR 4009, and HD 187399) were detected at the 3.3σ level or higher. For reasons discussed in this paper, HD 45314, π Aqr, κ Dra, and 48 Per are considered to be possible detections. The X-ray emission from λ Cas from late 1970 through early 1973 is discussed.

Type
VI. X-Ray Observations
Information
Symposium - International Astronomical Union , Volume 98: Be Stars , 1982 , pp. 353 - 357
Copyright
Copyright © Reidel 1982 

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