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Variability classes in the enigmatic black hole candidate GRS 1915+105 are known to be correlated with the variation of the Comptonizing Efficiency (CE) which is defined to be the ratio between the number of power-law (hard) photons and…

High Energy Astrophysical Phenomena · Physics 2015-08-11 Partha Sarathi Pal , Sandip K. Chakrabarti

Variability classes in the enigmatic black hole candidate GRS 1915+105 are known to be correlated with the variation of the Comptonizing Efficiency (CE) which is defined to be the ratio between the number of power-law (hard) photons and…

High Energy Astrophysical Phenomena · Physics 2015-10-29 Partha Sarathi Pal , Sandip K. Chakrabarti

A black hole accretion may have both the Keplerian and the sub-Keplerian components. We consider the most general accretion flow configuration, namely, two-component advective flow (TCAF) in which the Keplerian disk is immersed inside a low…

High Energy Astrophysical Phenomena · Physics 2014-06-17 Sudip Kumar Garain

From the study of X-ray light curve and color-color diagram of the low mass X-ray binary GRS 1915+105, observed by on board proportional counter array (PCA) of Rossi X-ray Timing Explorer (RXTE), we discover a new class of variability,…

High Energy Astrophysical Phenomena · Physics 2009-06-26 Mayukh Pahari , Sabyasachi Pal

Rectified flow and reflow procedures have significantly advanced fast generation by progressively straightening ordinary differential equation (ODE) flows. They operate under the assumption that image and noise pairs, known as couplings,…

Machine Learning · Computer Science 2024-11-04 Dogyun Park , Sojin Lee , Sihyeon Kim , Taehoon Lee , Youngjoon Hong , Hyunwoo J. Kim

We derive accretion flow properties of the transient black hole candidate (BHC) MAXI~J1543-564 using the RXTE data. We use Two-Component Advective Flow (TCAF) solution to fit the data of the very initial rising phase of outburst (from 2011…

High Energy Astrophysical Phenomena · Physics 2016-09-20 Debjit Chatterjee , Dipak Debnath , Sandip K. Chakrabarti , Santanu Mondal , Arghajit Jana

The Galactic transient X-ray binary MAXI~J1836-194 was discovered on 29th August 2011. Here we make a detailed study of the spectral and timing properties of its 2011 outburst using archival data of RXTE Proportional Counter Array…

High Energy Astrophysical Phenomena · Physics 2016-04-15 Arghajit Jana , Dipak Debnath , Sandip K. Chakrabarti , Santanu Mondal , Aslam Ali Molla

We report a detailed spectral study of Swift~J1357.2-0933 low-mass X-ray binary during its 2017 outburst using {\it Swift} and {\it NuSTAR} observations. We fit the data with two component advective flow (TCAF) model and power-law model. We…

High Energy Astrophysical Phenomena · Physics 2018-11-26 Santanu Mondal , Sandip K Chakrabarti

Galactic X-ray binary black hole candidate Swift~J1753.5-0127 was discovered on June 30 2005 by Swift/BAT instrument. In this paper, we make detailed analysis of spectral and timing properties of its 2005 outburst using RXTE/PCA archival…

High Energy Astrophysical Phenomena · Physics 2019-05-09 Dipak Debnath , Arghajit Jana , Sandip K. Chakrabarti , Debjit Chatterjee , Santanu Mondal

Based on the analysis of a small sample of BATSE and Konus gamma-ray bursts (GRBs) with know redshift it has been reported that the width of the autocorrelation function (ACF) shows a remarkable bimodal distribution in the rest-frame of the…

Astrophysics · Physics 2008-11-26 L. Borgonovo , F. Frontera , C. Guidorzi , E. Montanari , L. Vetere , P. Soffitta

Two component advective flow (TCAF) successfully explains spectral and timing properties of black hole candidates. We study the nature of photon trajectories in the vicinity of a Schwarzschild black hole and incorporate this in predicting…

High Energy Astrophysical Phenomena · Physics 2018-05-03 Arka Chatterjee , Sandip K. Chakrabarti , Himadri Ghosh

Outflows are common in many astrophysical systems. In the Two Component Advective Flow ({\fontfamily{qcr}\selectfont TCAF}) paradigm which is essentially a generalized Bondi flow including rotation, viscosity and cooling effects, the…

High Energy Astrophysical Phenomena · Physics 2021-10-20 Santanu Mondal , Sandip K. Chakrabarti

Nonlinear time series analysis has been widely used to search for signatures of low-dimensional chaos in light curves emanating from astrophysical bodies. A particularly popular example is the microquasar GRS 1915+105, whose irregular but…

High Energy Astrophysical Phenomena · Physics 2016-12-20 Manu Mannattil , Himanshu Gupta , Sagar Chakraborty

We report on the analysis of 100 ks INTEGRAL observations of the Galactic microquasar GRS 1915+105. We focus on INTEGRAL Revolution number 48 when the source was found to exhibit a new type of variability as preliminarily reported in…

We present a comprehensive X-ray study of four years of pointed RXTE observations of GRS 1915+105 in the chi-state. We interpret the behavior of the hard power law tail spectrum as coming from inverse Compton scattering of soft disk photons…

Astrophysics · Physics 2009-11-07 Arne Rau , Jochen Greiner

Recent simulations find that hot gas accretion onto compact accretors are often highly turbulent and diskless, and show power-law density profiles with slope $\alpha_\rho\approx-1$. These results are consistent with observational…

High Energy Astrophysical Phenomena · Physics 2023-07-19 Wenrui Xu

The light curve of the galactic micro-quasar GRS 1915+105 changes in at least thirteen different ways which are called classes. We present examples of the transitions from one class to another as observed by the IXAE instrument aboard the…

We report a comprehensive study on spectral and timing properties of hard X-ray dips uniquely observed in some so-called variability classes of the micro-quasars GRS 1915+105 and IGR J17091-3624. These dips are characterized by a sudden…

High Energy Astrophysical Phenomena · Physics 2015-06-17 Mayukh Pahari , J. S. Yadav , Jerome Rodriguez , Ranjeev Misra , Sudip Bhattacharyya , S. K. Pandey

We present a variability, color and morphology based classifier, designed to identify transients, persistently variable, and non-variable sources, from the Zwicky Transient Facility (ZTF) Data Release 11 (DR11) light curves of extended and…

Galactic black hole candidate MAXI J1910-057/Swift J1910.2-0546 was simultaneously discovered by MAXI/GSC and Swift/BAT satellites during its first outburst in 2012. We study the detailed spectral and temporal properties of the source in a…

High Energy Astrophysical Phenomena · Physics 2022-09-07 Sujoy Kumar Nath , Dipak Debnath , Kaushik Chatterjee , Arghajit Jana , Debjit Chatterjee , Riya Bhowmick