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Gamma-Ray Spectra & Variability of Cygnus X-1 Observed by BATSE

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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


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