Modelling the equatorial emission in the SS433 microquasar

Details Modelling the equatorial emission in the SS433 microquasar Modelling the equatorial emission in the SS433 microquasar

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012hell.conf...21s&link_type=abstract

10th Hellenic Astronomical Conference, Proceedings of the conference held at Ioannina, Greece, 5-8 September 2011. Edited by Io

Astronomy and Astrophysics

Astronomy

Scientific paper

The jets in the microquasar SS433 are modelled using a three-dimensional
relativistic hydrocode, with the aim of investigating the appearance of
equatorial radio emission. A dynamical mechanism is explored, including
the presence of an extended disc, whose role proves to be important in
producing the aforementioned emission.

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