Evidence for ultra-high-energy gamma-ray emission from the low-mass X-ray binary 2A 1822-37.1

Details Evidence for ultra-high-energy gamma-ray emission from the low-mass X-ray binary 2A 1822-37.1 Evidence for ultra-high-energy gamma-ray emission from the low-mass X-ray binary 2A 1822-37.1

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...346..151c&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 346, Nov. 1, 1989, p. 151-154. Research supported by the Australian Researc

Astronomy and Astrophysics

Astronomy

8

Cosmic Ray Showers, Gamma Ray Astronomy, Stellar Radiation, X Ray Binaries, Light Curve, Stellar Mass

Scientific paper

Evidence has been found for the observation of ultra-high-energy gamma
rays from the X-ray binary system 2A 1822-37.1. This source exhibits
emission over a broad range of binary phase which appears to change over
a period of years. These characteristics are similar to those observed
from the UHE source Cygnus X-3.

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