Accretion disk coronas in QSOs

Details Accretion disk coronas in QSOs Accretion disk coronas in QSOs

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aipc..254..268s&link_type=abstract

Testing the AGN paradigm. AIP Conference Proceedings, Volume 254, pp. 268-270 (1992).

Computer Science

Hydrodynamics, Radiation Mechanisms, Polarization

Scientific paper

Radiation pressure on gas in the hypothesized accretion disks of QSOs
will result in a corona. Electrons of 340 kev, equivalent to
Te~3×108 K, may result in a significant. Compton optical depth for
the implied mass loss rate. Comptonization of ultraviolet to 30 kev may
result in contradiction to observations.

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