Observation of gamma-rays from LMC X-4 above 10(16) eV

Details Observation of gamma-rays from LMC X-4 above 10(16) eV Observation of gamma-rays from LMC X-4 above 10(16) eV

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....1..247p&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 1 p 247-250 (SEE N85-33902 22-93)

Physics

Binary Stars, Cosmic Ray Showers, Extragalactic Radio Sources, Gamma Rays, Neutron Stars, X Ray Sources, Radio Emission, Signal To Noise Ratios

Scientific paper

Data from the University of Adelaide air shower array at Buckland Park taken over a three year period have been analysed to search for evidence of ultra-high energy γ-ray emission from neutron star binary X-ray sources having known orbital periods. The authors report the detection of UHE γ-rays from LMC X-4 above 1016eV, the first extragalactic object to be positively detected at these energies.

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