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The Radio X-Ray Correlation in Cygnus X-3 and Other Galactic Microquasars

Published online by Cambridge University Press:  22 February 2018

M. Choudhury  and
A. R. Rao
M. Choudhury
Affiliation:
Tata Institute of Fundamental Research, Mumbai-400005, India. (manojulu@tifr.res.in)
A. R. Rao
Affiliation:
Tata Institute of Fundamental Research, Mumbai-400005, India. (manojulu@tifr.res.in)

Extract

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Cygnus X-3, a Galactic X-ray binary, shows the presence of outflows in the form of radio jets. The SED in the X-ray band shows a complicated structure and evolution. We review some recent results of the long-term correlation of the radio and X-ray emissions, chiefly in the low (hard) states of the source. Comparing the results with those of other Galactic microquasars, we attempt to provide a consistent picture of the accretion — ejection mechanism in these sources.

Type
The Contributed Papers
Information
International Astronomical Union Colloquium , Volume 194: Compact binaries in the galaxy and beyond , 2004 , pp. 203
Copyright
Copyright © Instituto de astronomia/revista mexicana de astronomίa y astrofίsica 2004

References

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