High-energy neutrinos from Cygnus X-3

Details High-energy neutrinos from Cygnus X-3 High-energy neutrinos from Cygnus X-3

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...301..235b&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 301, Feb. 1, 1986, p. 235-239.

Astronomy and Astrophysics

Astrophysics

7

Energetic Particles, Gamma Rays, Neutrinos, Stellar Radiation, X Ray Binaries, Companion Stars, Luminosity, Particle Flux Density

Scientific paper

The high-energy neutrino flux from Cygnus X-3 is calculated on the basis of the binary model of the source. The possibility of observing such a flux through an excess of muons in small underground detectors is discussed. Constraints on the cosmic-ray luminosity of Cygnus X-3 are derived by comparing the expected neutrino flux with the gamma-ray observations of this source.

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