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 |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
3305303_306.PDF | 92.78 kB | Adobe PDF | View/Open |
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.