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

Ling, J. C.; Wheaton, A.; Wallyn, P.; Mahoney, W. A.; Paciesas, W. W.; Harmon, B. A.; Fishman, G. J.; Zhang, S. N.; Hua, X. M.

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