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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/784
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dc.contributor.authorChoudhury, M-
dc.date.accessioned2006-03-15T04:22:26Z-
dc.date.available2006-03-15T04:22:26Z-
dc.date.issued2005-09-
dc.identifier.citationBASI, Vol. 33, No. 3, pp. 303-306en
dc.identifier.urihttp://hdl.handle.net/2248/784-
dc.description.abstractMicroquasars 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-3en
dc.format.extent95005 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectaccretion- binariesen
dc.subjectclose - starsen
dc.subjectindividual (Cygnus X-3)- X-raysen
dc.subjectbinariesen
dc.titleHard X-ray and soft gamma ray properties of cosmic sourcesen
dc.typeArticleen
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