Abstract
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.
The National Radio Astronomy Observatory is operated by Associated Universities, Inc. under contract with the U.S. National Science Foundation.
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Hjellming, R.M. (1973). Radio Counterparts of X-ray Sources and X-ray Counterparts of Radio Stars. In: Bradt, H., Giacconi, R. (eds) X- and Gamma-Ray Astronomy. International Astronomical Union/Union Astronomique Internationale, vol 55. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-2585-0_8
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DOI: https://doi.org/10.1007/978-94-010-2585-0_8
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