4U 0115 + 63 - an energetic gamma ray binary pulsar

Details 4U 0115 + 63 - an energetic gamma ray binary pulsar 4U 0115 + 63 - an energetic gamma ray binary pulsar

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...151l...1c&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 151, no. 1, Oct. 1985, p. L1-L3. SERC-supported research.

Astronomy and Astrophysics

Astronomy

27

Gamma Ray Astronomy, Pulsars, X Ray Binaries, Light Curve, Radiant Flux Density, Stellar Luminosity, Stellar Rotation

Scientific paper

The emission of pulsed 1000 GeV γ-rays by the X-ray pulsar Her X-1 has recently been reported. A search for emission from an X-ray binary containing a pulsar with similar values of period, period derivative and luminosity has been successful. The sporadic X-ray binary 4U 0115+63 has been observed, with probability 10-5, to emit 1000 GeV γ-rays with a time averaged energy flux of 6×1035erg s-1.

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