Hydrodynamic Simulations of the SS433-W50 Complex

Details Hydrodynamic Simulations of the SS433-W50 Complex Hydrodynamic Simulations of the SS433-W50 Complex

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21334107g&link_type=abstract

American Astronomical Society, AAS Meeting #213, #341.07; Bulletin of the American Astronomical Society, Vol. 41, p.476

Astronomy and Astrophysics

Astronomy

Scientific paper

The compelling evidence for a connection between the microquasar SS433 and W50 the supernova remnant (SNR) has provoked much imagination for decades. There are still many unanswered questions: What was the nature of the progenitor of the black hole in SS433? What causes the evident re-collimation in SS433's jets? How recent is SS433's current precession state? What mass and energy contributions from a possible supernova explosion are required to produce W50? Here we present some of the results of our hydrodynamical simulations of the SS433-W50 system featuring: (i) the SNR evolution alone, and (ii) the SNR combined with interacting jets.

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