Study of instabilities in the interaction of jets with supernova remnants

Details Study of instabilities in the interaction of jets with supernova remnants Study of instabilities in the interaction of jets with supernova remnants

Nov 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998larm.confe..58v&link_type=abstract

"IX Latin American Regional IAU Meeting, "Focal Points in Latin American Astronomy", held in Tonantzintla, Mexico, Nov 9-13, 199

Astronomy and Astrophysics

Astronomy

Scientific paper

High resolution images from the system formed by the jets of SS433 and the old SNR W50 reveals the existence of a "chimney" of synchrotron radiation, which is located near the head of the eastern jet. This chimney is found at approximately 50 pc from the origin, where the jet pushes the interstellar medium, developing an elongated cavity. We analyze the different hydrodynamic instabilities that occur in this scenario.

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