With frequent flaring activity of its relativistic jets, Cygnus X‐3 (Cyg X‐3) is one of the most
active microquasars and is the only Galactic black hole candidate with confirmed high …

There is increasing evidence that active galactic nucleus (AGN) feedback is important in the
energetics of cooling flows in galaxies and galaxy clusters. It is possible that, in most cooling …

We study the soft X-ray variability of Cygnus X-3. By combining data from the All-Sky Monitor
and Proportional Counter Array instruments on the RXTE satellite with EXOSAT/Medium …

The wide-band X-ray spectra of the high-mass X-ray binary Cyg X-3 exhibit a pivoting
behavior in the" low"(as well as" hard") state, correlated to the radio emission. The timescale …

We have re-analysed archival RXTE data of the X-ray binary Cygnus X− 3 with a view to
investigate the timing properties of the source. As compared to previous studies, we use an …

Variation of mass supply rate from the companion can be smeared out by viscous processes
inside an accretion disk. Hence, by the time the flow reaches the inner edge, the variation in …

We discuss the origin of superluminal radio jets in Black hole X-ray binaries with relativistic
radio jets in our Galaxy popularly known as microquasars. We classify the relativistic …

Stellar companion of a black hole orbiting in an eccentric orbit will experience modulating
tidal force with a periodicity same as that of the orbital period. This, in turn, would modulate …