Modelling the equatorial activity in SS433

Details Modelling the equatorial activity in SS433 Modelling the equatorial activity in SS433

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aipc..848..442s&link_type=abstract

RECENT ADVANCES IN ASTRONOMY AND ASTROPHYSICS: 7th International Conference of the Hellenic Astronomical Society. AIP Conferenc

Astronomy and Astrophysics

Astrophysics

Hydrodynamics, Mass Loss And Stellar Winds

Scientific paper

The jets in SS433 were modelled using a two-dimensional classical hydrocode and a dynamical mechanism was suggested to explain the observed equatorial radio features in SS433. The modelling provided constraints to a number of jet and stellar wind parameters for the jet-wind system. An ambient density falling off away from the jet base was found to offer the best results for enhancing the equatorial region activity.

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