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 |
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dc.format.mimetype |
application/pdf |
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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 |