UHE particle production in close binary systems

Details UHE particle production in close binary systems UHE particle production in close binary systems

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....2..296h&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 2 p 296-299 (SEE N85-34006 22-93)

Physics

Cosmic Ray Showers, Cygnus Constellation, Flux (Rate), Gamma Rays, Charged Particles, Energy Spectra, X Ray Sources

Scientific paper

Cygnus X-3 appears to generate so much power in the form of charged particles of up to approx 10 to the 17th power eV that the galaxy may need approx 1 such source on average to maintain its flux of ultra high energy cosmic rays. Accreting gas must supply the energy, and in a surprisingly ordered form, if it is correct to use a Vest-rand-Eichler model for radiation of gammas, modified by the introduction of an accretion wake. Certain relationships between 10 to the 12th power eV and 10 to the 15th power gamma rays are expected.

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