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Spectro-temporal signatures of accretion flows around Galactic Black Holes
A system of two stars in which one is a black hole (BH) is referred to as a black hole
binary (BHB). In a BHB, it is possible to have mass transfer from the secondary star
(companion star) to the primary black hole. ...
Nonlinear and Geometric Properties of Accreting Compact Sources Based on Spectral and Timing Analyses
We study the spectro-temporal properties of the black hole X-ray binaries (BHXBs) GRS 1915+105
and IGR J17091-3624 with data from RXTE, Chandra and XMM-Newton. From the analysis
result, we propose models of accretion ...
Effect of AGN on the ISM of their hosts: A multi-wavelength perspective
Active Galactic Nuclei (AGN) are among the high luminosity (1011 − 1014 L⊙ ) sources in the
observable Universe, believed to be powered by the accretion of matter onto supermassive
black holes (SMBHs; 105 − 1010 M⊙ ) at ...

