Thermal Comptonization models for gamma-ray emission from black-hole sources.

Details Thermal Comptonization models for gamma-ray emission from black-hole sources. Thermal Comptonization models for gamma-ray emission from black-hole sources.

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989nyasa.571..513d&link_type=abstract

14. Texas Symposium on Relativistic Astrophysics, p. 513 - 521

Astronomy and Astrophysics

Astrophysics

2

Gamma-Ray Sources: Black Holes, Gamma-Ray Sources: Radiation Mechanisms, Gamma-Ray Sources: Compton Scattering

Scientific paper

The list of black-hole candidates detected at gamma-ray energies includes the Galactic sources Cygnus X-1 and the Galactic Center, and the extragalactic sources Cen A, NGC 4151, MCG 8-11-11, and 3C 273. The luminosity of these objects peaks in the photon energy range 0.1 - 10 MeV and dominates the total energy output in the observable wave bands. In this review, successes and limitations of thermal Comptonization models for the high-energy emission of black-hole sources are considered.

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