Physics – High Energy Physics
Scientific paper
Jan 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1206..312k&link_type=abstract
ASTROPHYSICS AND COSMOLOGY AFTER GAMOW: Proceedings of the 4th Gamow International Conference on Astrophysics and Cosmology Afte
Physics
High Energy Physics
Jets, Stellar Coronae, Accretion Disks, X-Ray Binary Stars, Jets And Bursts, Galactic Winds And Fountains, Stellar Atmospheres, Radiative Transfer, Opacity And Line Formation, Accretion And Accretion Disks, X-Ray Binaries
Scientific paper
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.
Bisnovatyi-Kogan Gennadi S.
Cherepashchuk Anatol M.
Krivosheyev Yu. M.
Postnov Konstantin A.
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