dc.contributor.author | Ling, J. C. | en_US |
dc.contributor.author | Wheaton, A. | en_US |
dc.contributor.author | Wallyn, P. | en_US |
dc.contributor.author | Mahoney, W. A. | en_US |
dc.contributor.author | Paciesas, W. W. | en_US |
dc.contributor.author | Harmon, B. A. | en_US |
dc.contributor.author | Fishman, G. J. | en_US |
dc.contributor.author | Zhang, S. N. | en_US |
dc.contributor.author | Hua, X. M. | en_US |
dc.date.accessioned | 2004-10-01T06:08:27Z | |
dc.date.available | 2004-10-01T06:08:27Z | |
dc.date.issued | 1996 | en_US |
dc.identifier.clearanceno | 96-1667 | en_US |
dc.identifier.uri | http://hdl.handle.net/2014/27616 | |
dc.description.abstract | We present new BATSE Earth occultation observations of the 25 keV-1.8 MeV spectrum and variability of Cygnus X-1 made between August 1993 and May 1994. We observed that the normal soft gamma-ray spectrum (gamma2) of Cygnus X-1 has two components: a Comptonized part seen below 30keV, and a high-energy tail in the 0.3-2 MeV range. | en_US |
dc.format.extent | 1575622 bytes | |
dc.format.mimetype | application/pdf | |
dc.language.iso | en_US | |
dc.subject.other | Black holes gamma rays occultation | en_US |
dc.title | Gamma-Ray Spectra & Variability of Cygnus X-1 Observed by BATSE | en_US |