Hercules X-1: Pulsed gamma-rays detected above 150 GeV

Details Hercules X-1: Pulsed gamma-rays detected above 150 GeV Hercules X-1: Pulsed gamma-rays detected above 150 GeV

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....1..119c&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 1 p 119-122 (SEE N85-33902 22-93)

Computer Science

Binary Stars, Cosmic Ray Showers, Gamma Ray Bursts, Infrared Radiation, Optical Properties, Rates (Per Time), Extraterrestrial Radiation, Galactic Radiation, Uhuru Satellite

Scientific paper

The 1.24 second binary pulsar Her X-1, first observed in X-rays in 1971 by UHURU has now been seen as a sporadic gamma ray source from 1 TeV up to at least 500 TeV. In addition, reprocessed optical and infrared pulses are seen from the companion star HZ Herculis. Thus measurements of the Her X-1/HZ Herculis system span 15 decades in energy, rivaling both the Crab pulsar and Cygnus X-3 in this respect for a discrete galactic source.

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