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MG12 - Talk detail
 

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 Participant 

Krivosheyev, Yuri

Institution

Space Research Institute (IKI) of Russian Academy of Sciences  - Profsoyuznaya str. - Moscow - - Russia

Session

Talk

Abstract

BHT3

Unique Black Hole Source SS433: Monte-Carlo modelling

We propose a physical model of the galactic superaccreting microquasar SS433 X-ray emitting region that includes thermal emission from the accretion disk, jets and hot corona where the photons of diff erent origin are comptonized. We develop a Monte-Carlo technique to calculate X-ray continuum spectra of comptonized thermal plasma in arbitrary geometry and apply it to describe the broadband X-ray continuum observed by INTEGRAL. From comparison with INTEGRAL observations, we estimate physical parameters of the complex X-ray emitting region in SS433. Also, model spectra for di fferent object viewing angles are presented.

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