Hard X-ray and soft gamma ray properties of cosmic sources

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/784

Title:	Hard X-ray and soft gamma ray properties of cosmic sources
Authors:	Choudhury, M
Keywords:	accretion- binaries close - stars individual (Cygnus X-3)- X-rays binaries
Issue Date:	Sep-2005
Publisher:	Astronomical Society of India
Citation:	BASI, Vol. 33, No. 3, pp. 303-306
Abstract:	Microquasars provide a unique laboratory to study the accretion process in a compact object, coupled to the ejection of matter in the form of jets. In this thesis we provide a phenomenological perspective on the accretion- ejection mechanism based on the multi-wavelength observational features cov- ering long term evolution of various sources exhibiting apparently diverse types of characteristics, with special emphasis on the enigmatic X-ray binary system Cygnus X-3
URI:	http://hdl.handle.net/2248/784
Appears in Collections:	BASI Publications

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