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Speaker |
Krivosheyev, Yuri |
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Co-autors |
G.S. Bisnovatyi-Kogan, A.M. Cherepashchuk, K.A. Postnov |
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Talk Title |
Unique Black Hole Source SS433: Monte-Carlo modelling |
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Abstract |
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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Talk view |
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