Generation of infrared synchrotron radiation in the accretion disk coronas in X-ray binary systems

Details Generation of infrared synchrotron radiation in the accretion disk coronas in X-ray binary systems Generation of infrared synchrotron radiation in the accretion disk coronas in X-ray binary systems

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15..513i&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 15, June 1989, p. 513-518. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

Accretion Disks, Infrared Astronomy, Stellar Coronas, Synchrotron Radiation, X Ray Binaries, Electric Fields, Electron Acceleration, Electron Energy, Relativistic Electron Beams

Scientific paper

The generation of synchrotron radiation from ultrarelativistic electrons accelerated by the electric field of a differentially rotating accretion disk is considered. It is shown that infrared synchrotron radiation may be generated by electrons with energies up to gamma = 30-200 in the near corona of a magnetized disk. The admissible values of concentrations of thermal and relativistic electrons in the emitting regions are estimated.

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