The 4U 0115+63: Another energetic gamma ray binary pulsar

Details The 4U 0115+63: Another energetic gamma ray binary pulsar The 4U 0115+63: Another energetic gamma ray binary pulsar

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....1..251c&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 1 p 251-254 (SEE N85-33902 22-93)

Mathematics

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1

Binary Stars, Cosmic Ray Showers, Pulsars, Radio Emission, X Ray Sources, Luminosity, Magnetic Fields, Time Measurement, X Ray Telescopes

Scientific paper

Following the discovery of Her X-1 as a source of pulsed 1000 Gev X-rays, a search for emission from an X-ray binary containing a pulsar with similar values of period, period derivative and luminosity was successful. The sporadic X-ray binary 4U 0115-63 has been observed, with probability 2.5 x 10 to the minus 6 power ergs/s to emit 1000 GeV gamma-rays with a time averaged energy flux of 6 to 10 to the 35th power.

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