Models of unsaturated Compton disks around supermassive black holes

Details Models of unsaturated Compton disks around supermassive black holes Models of unsaturated Compton disks around supermassive black holes

Nov 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979mnras.189..421l&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 189, Nov. 1979, p. 421-432.

Astronomy and Astrophysics

Astronomy

38

Astronomical Models, Black Holes (Astronomy), Galactic Nuclei, Quasars, X Ray Spectra, Active Galactic Nuclei, Cooling, Coronas, High Energy Electrons, Optical Thickness, Rotating Disks, X Ray Sources

Scientific paper

Two inverse-Compton disk models for the hard X-ray spectra of quasi-stellar objects and active galactic nuclei are studied and compared. One is a slightly generalized version of the Shapiro, Lightman and Eardley optically thin disk model, and the other is a conduction-stabilized Corona model. Observational distinctions between the two models are discussed.

Affiliated with

Also associated with

No associations

Rating

Models of unsaturated Compton disks around supermassive black holes does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Models of unsaturated Compton disks around supermassive black holes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Models of unsaturated Compton disks around supermassive black holes will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-975412