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A search for TeV emission from cygnus X-3

  • K. S. O'Flaherty
  • , M. F. Cawley
  • , D. J. Fegan
  • , R. C. Lamb
  • , M. J. Lang
  • , D. A. Lewis
  • , M. Punch
  • , P. T. Reynolds
  • , G. Vacanti
  • , T. C. Weekes
  • University College Dublin
  • St. Patrick's College
  • Iowa State University
  • Harvard & Smithsonian
  • Whipple Observatory
  • Université Paris Diderot

Research output: Contribution to a Journal (Peer & Non Peer) › Article › peer-review

23 Citations (Scopus)

Abstract

Cygnus X-3 has been observed during 1988-1990 by the Whipple Observatory collaboration using the 109 pixel high-resolution γ-ray imaging telescope. The data recorded has been analyzed to search for (a) steady emission of TeV γ-rays, (b) 4.8 hr modulation of the γ-ray light curve, and (c) periodic emission at 12.59 ms. No evidence is found for emission based on these searches. The upper limit (3 a) for long-term steady emission is 3.5 × 10-12 photons cm-2 s-1, a factor of 10 below fluxes reported a decade ago for this energy.

Original languageEnglish
Pages (from-to)674-678
Number of pages5
JournalAstrophysical Journal
Volume396
Issue number2
DOIs
Publication statusPublished - 1992

Keywords

  • Gamma rays: observations
  • Stars: individual (Cyg X-3)

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