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Are Classical Be Stars Sources of Hard X-Rays?
Published online by Cambridge University Press: 14 August 2015
Abstract
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.
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- VI. X-Ray Observations
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- Copyright © Reidel 1982
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