High Resolution Radio Images of X-ray Binary, Cygnus X-3, after a Large Radio Flare in April 2000

Details High Resolution Radio Images of X-ray Binary, Cygnus X-3, after a Large Radio Flare in April 2000 High Resolution Radio Images of X-ray Binary, Cygnus X-3, after a Large Radio Flare in April 2000

Oct 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000head....5.2301m&link_type=abstract

American Astronomical Society, HEAD Meeting #5, #23.01; Bulletin of the American Astronomical Society, Vol. 32, p.1215

Astronomy and Astrophysics

Astronomy

Scientific paper

Cygnus X-3 is one of the growing number of X-ray binaries known to have relativistic outflows. In Cyg X-3 these outflows occur during and after large flares in the radio which are always associated with activity in the hard and soft X-ray. On 1 April 2000 and for several days afterwards, Cygnus experienced several large (>10 Jy) flares. Here we present high resolution VLBA images of Cyg X-3 1, 2, 3, 5, 6, and 20 days after the peak of the first large flare. We will compare these images to previous VLBA observations in February 1997, which showed a curved one-sided relativistic jet.

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