Jets, corona and accretion disk in the black holesource SS433: Monte-Carlo simulations

摘要

We propose a physical model of the X-ray emitting region of the Galactic microquasar SS433 that includes thermal emission from the accretion disk, jets and hot corona where the photons of different origin are comptonized. We have employed a Monte-Carlo technique to calculate X-ray continuum spectra of comptonized thermal plasma and applied it to describe the broadband X-ray continuum of SS433 observed by INTEGRAL. From comparison with INTEGRAL observations, we estimate physical parameters of the X-ray emitting region in SS433 and present model spectra for different viewing angles of the object.