A reevaluation of self-absorption of TeV photon flux from Cygnus X-3

Details A reevaluation of self-absorption of TeV photon flux from Cygnus X-3 A reevaluation of self-absorption of TeV photon flux from Cygnus X-3

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...339..382m&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 339, April 1, 1989, p. 382-385.

Astronomy and Astrophysics

Astronomy

Cygnus Constellation, Infrared Radiation, Photon Beams, Radiative Transfer, Self Absorption, X Ray Binaries, Electron-Positron Pairs, Gamma Ray Astronomy, Radiation Distribution

Scientific paper

The attenuation factor for the absorption of TeV gamma-rays from Cygnus
X-3 by its own IR radiation field is examined. The spectrum of IR
photons is discussed as well as optical depth, the attenuation of TeV
flux, and the realistic yield function. The typical PeV photon yield
functions were found to have a Gaussian type profile.

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