Research Accomplished

The above mentioned informations motivates us to formulate a simultaneous inflow-outflow solution for explaining the hydrodynamic origin of astrophysical outflows from sources powered by accreting compact objects and to compute the mass outflow rate only in terms of accretion parameters. Our initial work (Das, 1999, Monthly Notices of the Royal Astronomical Society, 308, 201; Das & Chakrabarti, 1999, Classical and Quantum Gravity. 16, 3879; Das, 2000, Monthly Notices of the Royal Astronomical Society 318, 294; Das, 2001, Astronomy & Astrophysics 376, 697; Das, 2001, Astrophysics and Space Science 276, 267) demonstrated how accretion powered hydrodynamic jet/outflow can be generated from the close vicinity of galactic and extra galactic black hole candidates.