085319

We propose an 80 ks high-spatial resolution Chandra-HRC-I observation of the MWC 560 symbiotic interacting binary system comma as a follow-up to the 2016 Chandra discovery of an extended jet-outflow. When combined with the joint HST imaging and XMM spectra comma we will obtain a comprehensive picture of the central source and the dynamic jet-outflow from as close as few hundred AU from its source comma to the region of its interaction with the circumbinary environment into which the jet propagates. We will determine its evolution and origin comma including association with powerful past outbursts in the system.