Titlebook: Exploring the Universe: From Near Space to Extra-Galactic; A Collection of Rese Banibrata Mukhopadhyay,Sudipta Sasmal Conference proceeding

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Hydrogen Production from Recycled Gases,tional wave signal emitted from such systems. On the other hand, by studying the emitted gravitational wave signals profile, one could infer about the nature of the accretion disk, which has been, till date, done only by observing the electro-magnetic signals coming from it. This multi-messenger ast

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Aleksander Koll,Peter Wolschannly, we calculate the critical values of both viscosity and accretion rate that cater shocks. We continue the search of shocked accretion solutions for two-temperature flow and obtain such solutions for the first time in the literature. Finally, we discuss the possible origin of mass loss from the ac

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Han Myoung Lee,N. Jiten Singh,Kwang S. Kiman 0.008, all sources were categorized in hard spectral state. When it was in the ranges 0.008–0.035 and 0.035–0.01, hard and soft intermediate states were observed respectively. Soft spectral state would be expected for any larger values of . in the sub-Keplerian component. Thus the concept of visc

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Hydrogen: The Ultimate Energy Sourcee an advective halo. We believe that, for the first time, our results are able to simulate the two-component advective flow dynamics during an entire X-ray outburst of a black hole candidate. Also, we see, the hysteresis effect of an outburst is caused mainly for the difference in the time duration

Dislocation

https://doi.org/10.1007/978-0-85729-136-3cularly true for weakly viscous, low angular momentum transonic or advective discs. We focus our study to the trajectories of toroidal flux tubes inside a geometrically thick flow which undergoes a centrifugal force supported shock and also the effects of these flux tubes on the dynamics of the infl

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