Neutral particle emission from the X-ray binary 2A 1822-37 at energies above 10 exp 17 eV

Details Neutral particle emission from the X-ray binary 2A 1822-37 at energies above 10 exp 17 eV Neutral particle emission from the X-ray binary 2A 1822-37 at energies above 10 exp 17 eV

Feb 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...255..167c&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 255, no. 1-2, p. 167-170.

Astronomy and Astrophysics

Astrophysics

12

Binary Stars, Gamma Ray Spectra, Muons, X Ray Stars, Arrays, Cosmic Ray Showers, Energy Spectra

Scientific paper

An examination of data recorded by the Sydney University Giant Air shower Recorder gives evidence for the detection of neutral particles from the X-ray binary 2A 1822-37.1 at energies above 10 exp 17 eV. We estimate a flux of 2 x 10 exp -11/sq m/s above 1.8 x 10 exp 17 eV. It is unlikely that the neutral primary particles are gamma-rays since there is a strong signal present in the array detectors, which predominately detect muons. The phase dependence of the signal is similar to that found at lower energies from the same source.

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