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

dc.contributor.author	Choudhury, M
dc.date.accessioned	2006-03-15T04:22:26Z
dc.date.available	2006-03-15T04:22:26Z
dc.date.issued	2005-09
dc.identifier.citation	BASI, Vol. 33, No. 3, pp. 303-306	en
dc.identifier.uri	http://hdl.handle.net/2248/784
dc.description.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	en
dc.format.extent	95005 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	accretion- binaries	en
dc.subject	close - stars	en
dc.subject	individual (Cygnus X-3)- X-rays	en
dc.subject	binaries	en
dc.title	Hard X-ray and soft gamma ray properties of cosmic sources	en
dc.type	Article	en