Theoretical Modelling of X-Ray Emissions from Black Hole Accretion Disks

Details Theoretical Modelling of X-Ray Emissions from Black Hole Accretion Disks Theoretical Modelling of X-Ray Emissions from Black Hole Accretion Disks

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008asthe.101..717k&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 101, No. 12, p. 717 - 726 (2008)

Physics

Scientific paper

Active galactic nuclei and X-ray binaries are considered to be energized by black hole accretion disks. X-ray spectra of accreting black holes have been the most important probes of the physics working at the region close to the black hole, such as the space-time structure, the dynamics of accretion flows, radiative processes, and so on. The authors discuss the physics of the accreting black hole system including the cold disk and hot corona, and the X-ray emission features predicted such systems.

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