Cygnus X-3 and egret gamma-ray observations

  • M. Mow*
  • , D. L. Bertsch
  • , B. L. Dlngus
  • , J. A. Esposito
  • , C. E. Fichtel
  • , S. D. Hunter
  • , G. Kanbach
  • , D. A. Kniffen
  • , Y. C. Lin
  • , J. R. Mattox
  • , H. A. Mayer-Hasselwander
  • , P. F. Michelson
  • , C. Von Montigny
  • , R. Mukherjee
  • , P. L. Nolan
  • , P. V. Ramanamurthy
  • , E. Schneid
  • , P. Sreekumar
  • , D. J. Thompson
  • *Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

Abstract

The Energetic Gamma Ray Experiment Telescope (EGRET) aboard the Compton Gamma Ray Observatory observed the Cygnus region in 14 different viewing periods during 1991 May to 1994 July. We present here our results on unpulsed and pulsed emissions of gamma rays at E > 50 MeV from Cyg X-3. While we detect a gamma-ray source consistent with the position of Cyg X-3, there was no evidence for the characteristic ~4.79 hr periodicity observed in X-rays and infrared.

Original languageEnglish
Pages (from-to)842-846
Number of pages5
JournalAstrophysical Journal
Volume476
Issue number2 PART I
DOIs
Publication statusPublished - 1997

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

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