Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.398d&link_type=abstract
Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:
Astronomy and Astrophysics
Astrophysics
Scientific paper
Active galaxies and quasars are believed to harbour black holes at their centres and at the same time produce cosmic radio jets through which immense amount of matter and energy are ejected out of the core of the galaxy. In our work we compute the mass outflow rates from advective accretion disks around black holes which, we believe, could explain the origin of jet formation from AGNs & QSOs. These computations are done using combinations of exact transonic inflow and outflow solutions which may or may not form standing shock waves. Our work for the first time connects the accretion type and wind type topologies self consistently. All our previous considerations are also valid for micro-quasars such as compact X ray binaries. Our result, in general, matches with numerical simulation works and successfully points out to non-steady behaviors which may almost evacuate the disk and produce quiescence states.
Chakrabarti Sandip K.
Das Tapas Kumar
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