Search forγrays aboveeV from Cygnus X-3 during the June and July 1989 radio outbursts
- 20 November 1989
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review Letters
- Vol. 63 (21) , 2329-2332
- https://doi.org/10.1103/physrevlett.63.2329
Abstract
We have looked for γ-ray emission above 100 TeV from the binary x-ray source Cygnus X-3 during a period of intense radio emission in the summer of 1989. We find no evidence for excess air showers from the direction of the source and the muon content of air showers from this direction is the same as that of ordinary cosmic rays. The flux of γ rays from Cygnus X-3 with energies exceeding 2.1× eV is <5.5× (90% C.L.).
Keywords
This publication has 10 references indexed in Scilit:
- Evidence for-eV Neutral Particles from the Direction of Cygnus X-3Physical Review Letters, 1989
- Time delay of the PeV gamma ray burst after the October 1985 radio flare of Cygnus X-3Nature, 1988
- Hadron Structure of High-Energy PhotonsPhysical Review Letters, 1988
- Electromagnetic component of–-eV air showersPhysical Review D, 1988
- Is Cygnus X-3 a monoenergetic 1017 eV accelerator?Nature, 1984
- Analysis methods for results in gamma-ray astronomyThe Astrophysical Journal, 1983
- Gamma-rays and the production of energetic electrons in enshrouding material - A model for the quiescent radio emission from Cygnus X-3The Astrophysical Journal, 1983
- Upper limit of peak areaNuclear Instruments and Methods in Physics Research, 1983
- A model for the radio outbursts of Cygnus X-3The Astrophysical Journal, 1976
- Cosmic Ray ShowersAnnual Review of Nuclear Science, 1960