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Radio Counterparts of X-Ray Sources and X-Ray Counterparts of Radio Stars

Published online by Cambridge University Press:  14 August 2015

R. M. Hjellming
R. M. Hjellming*
Affiliation:
National Radio Astronomy Observatory∗, Green Bank, West Virginia, U.S.A.

Abstract

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Some of the implications of the data on radio counterparts of X-ray sources are discussed. Data on the radio counterpart of Cyg X-3 is compared with the data on the radio star β Persei (Algol), to show that similar radio emission mechanisms are involved. The data for such radio stars not yet known as X-ray sources imply that such objects should be transient X-ray sources.

Type
Part I: Galactic Sources
Information
Symposium - International Astronomical Union , Volume 55: X- and Gamma-Ray Astronomy , 1973 , pp. 98 - 104
Copyright
Copyright © Reidel 1973 

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