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Radio Emission From Strong X-Ray Sources

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Radio Stars

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 116))

Abstract

We review the properties of some of the radio sources associated with very energetic stellar systems that are also strong x-ray sources. Extended lobes of radio emission are seen in Sco X-1, SS433, and Cyg X-3, with the latter two showing regular or intermittent indications of expanding structures with velocities of the order of 0.3c. Some of the observations of these and other radio-emitting x-ray sources are summarized. A working model of accretion-disk outflows resulting in jets that expand like “cylindrical” supernovae is discussed as an explanation for the production of relativistic particles and fields in SS433. The ubiquity of jets and strong synchrotron sources in these and other mass-outflow objects is discussed.

The National Radio Astronomy Observatory is operated by Associated Universities, Inc., under contract with the National Science Foundation.

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Author information

Authors and Affiliations

  1. National Radio Astronomy Observatory, Socorro, NM, 87801, USA

    R. M. Hjellming

  2. Naval Research Laboratory, E.O. Hulburt Center for Space Research, Washington, D.C., 20375, USA

    K. J. Johnston

Authors
  1. R. M. Hjellming
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  2. K. J. Johnston
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Editor information

Editors and Affiliations

  1. National Radio Astronomy Observatory, Socorro, New Mexico, USA

    Robert M. Hjellming

  2. New Mexico Institute of Mining and Technology, Socorro, New Mexico, USA

    David M. Gibson

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© 1985 D. Reidel Publishing Company

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Hjellming, R.M., Johnston, K.J. (1985). Radio Emission From Strong X-Ray Sources. In: Hjellming, R.M., Gibson, D.M. (eds) Radio Stars. Astrophysics and Space Science Library, vol 116. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-5420-5_42

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  • DOI: https://doi.org/10.1007/978-94-009-5420-5_42

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-8892-3

  • Online ISBN: 978-94-009-5420-5

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