Cygnus X‐3 and EGRET Gamma‐Ray Observations
The Astrophysical Journal1997Vol. 476(2), pp. 842–846
Citations Over TimeTop 10% of 1997 papers
M. Mori, D. L. Bertsch, B. L. Dingus, 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. J. Schneid, P. Sreekumar, D. J. Thompson
Abstract
0!rQ1The 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.
Related Papers
- → The NMSU 1 m Telescope at Apache Point Observatory(2010)39 cited
- → VST project: mechanical design optimization(2003)2 cited
- → First Telescope of the Russian–Cuban Observatory(2022)2 cited
- → VST project: drive system design and strategies for performance optimization(2003)1 cited
- Visual supernova searching with the 40-inch telescope at Siding Spring Observatory.(1996)