The post-outburst radio evolution of Cygnus X-3

Abstract

Cygnus X-3 is one of the most famous Galactic relativistic jet sources, often undergoing flares to 1 Jy or more. Here we present VLBA imaging at 15 and 22 GHz after the September 2001 outburst and contrast the one-sided nature of the VLBI jets with the two-sided jet seen in VLA images of this source

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