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

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

Sep 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005basi...33..303c&link_type=abstract

Bulletin of the Astronomical Society of India, vol. 33, Issue 3, p.303

Mathematics

Logic

Accretion, Binaries : Close, Stars : Individual (Cygnus X-3), X-Rays : Binaries

Scientific paper

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.

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