Quenched Radio Emission in Cygnus X-3

Details Quenched Radio Emission in Cygnus X-3 Quenched Radio Emission in Cygnus X-3

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aas...19111005w&link_type=abstract

American Astronomical Society, 191st AAS Meeting, #110.05; Bulletin of the American Astronomical Society, Vol. 29, p.1388

Astronomy and Astrophysics

Astronomy

Scientific paper

Monitoring of X-ray binaries at 2.25 and 8.3 GHz with the Green Bank Interferometer has recorded quenched radio emission during active periods in Cygnus X-3 on a timescale of days to weeks prior to major flares. This is too long to be explained as self-absorption in the expanding synchrotron model, but may be attributed to instabilities in the environment of jet formation during periods of enhanced accretion.

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