Model' tsentral'nogo rentgenovskogo istochnika v aktivnykh galakticheskikh yadrakh

Details Model' tsentral'nogo rentgenovskogo istochnika v aktivnykh galakticheskikh yadrakh Model' tsentral'nogo rentgenovskogo istochnika v aktivnykh galakticheskikh yadrakh

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002pobeo..74..185s&link_type=abstract

Publications of the Astronomical Observatory of Belgrade (ISSN 0373-3742), No. 74, p. 185 - 188 (2002). In: Invited lectures and

Physics

Radio Galaxies, Quasars, Disk Accretion, Black Holes

Scientific paper

Disk accretion mechanism onto massive black holes in nuclei of radiogalaxy M82 and quasar 3C 273 is considered. Basing on the X-ray spectra and black hole mass estimations, accretion rates and inner boundary radii are determined. Obtained luminosity of 3C 273 quasar at ν > 1015Hz doesn't exceed the Eddington limit. Possible disk feeding sources and accretion conditions are analysed. Black hole mass and galactic nuclear medium influence on accretion properties is determined.

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