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Galactic transient black hole candidate (BHC) MAXI~J1836-194 was discovered on 2011 Aug 30, by MAXI/GSC and Swift/BAT. The source activity during this outburst was continued for ~3 months before entering into the quiescent state. It again…

高能天体物理现象 · 物理学 2020-05-20 Arghajit Jana , Dipak Debnath , Sandip K. Chakrabarti , Debjit Chatterjee

Galactic black hole candidate (BHC) XTE~J1118+480 during its 2000 outburst has been studied in a broad energy range using the archival data of PCA and HEXTE payloads of {\it Rossi X-ray Timing Explorer}. Detailed spectral and temporal…

高能天体物理现象 · 物理学 2019-05-09 Debjit Chatterjee , Dipak Debnath , Arghajit Jana , Sandip K. Chakrabarti

We study transient Galatic black hole candidate MAXI~J1836-194 during its 2011 outburst using RXTE/PCA archival data. 2.5-25~keV spectra are fitted with Two Component Advective Flow (TCAF) model fits file as an additive table local model in…

高能天体物理现象 · 物理学 2019-02-27 Arghajit Jana , Dipak Debnath , Sandip K. Chakrabarti , Santanu Mondal , Aslam Ali Molla , Debjit Chatterjee

The 2015 Outburst of V404 Cygni is an unusual one with several X-ray and radio flares and rapid variation in the spectral and timing properties. The outburst occurred after $26$ years of inactivity of the black hole. We study the accretion…

高能天体物理现象 · 物理学 2020-06-08 Arghajit Jana , Jie-Rou Shang , Dipak Debnath , Sandip K. Chakrabarti , Debjit Chatterjee , Hsiang-Kuang Chang

We carry out a detailed study of the spectral and the timing properties of the stellar-mass black hole candidate XTE J1752-223 during its 2009-10 outburst using RXTE PCA data in the $2.5-25$ keV energy range. Low frequency quasi-periodic…

高能天体物理现象 · 物理学 2020-02-12 Kaushik Chatterjee , Dipak Debnath , Debjit Chatterjee , Arghajit Jana , S. K. Chakrabarti

We present detailed timing and spectral studies of the black hole candidate MAXI J0637$-$430 during its 2019-2020 outburst using observations with the {\em Neutron Star Interior Composition Explorer (NICER)} and the {\em Neil Gehrels Swift…

We report on the detection and subsequent X-ray monitoring of the new Galactic black hole candidate MAXI J1535-571 with the MAXI/GSC. Afterthe discovery on 2017 September 2 made independently with MAXI and the Swift/BAT, the source…

We present a broadband spectral and timing study of the black hole candidate MAXI J1803-298 during its 2021 outburst using simultaneous observations from NICER, NuSTAR, and Insight-HXMT. The combined multi-instrument coverage allows us to…

高能天体物理现象 · 物理学 2026-05-14 Kaushik Chatterjee , Sujoy K. Nath

We analyzed two observations of the low-mass black hole X-ray binary MAXI J1348-630 from Nuclear Spectroscopic Telescope Array (NuSTAR) during low hard state and hard intermediate state in the 2019 outburst. The reflection components are…

高能天体物理现象 · 物理学 2023-04-27 Hanji Wu , Wei Wang , Na Sai

We present the results of our quasi-simultaneous radio, sub-mm, infrared, optical and X-ray study of the Galactic black hole candidate X-ray binary MAXI J1836-194 during its 2011 outburst. We consider the full multi-wavelength spectral…

高能天体物理现象 · 物理学 2015-06-18 T. D. Russell , R. Soria , J. C. A. Miller-Jones , P. A. Curran , S. Markoff , D. M. Russell , G. R. Sivakoff

MAXI J1348-630 as a low-mass black hole binary system in the Galaxy showed an X-ray outburst in 2019. We analyzed the Insight-HXMT spectral data in the low hard state (LHS) and intermediate state (IS) during the outburst from MJD 58510 to…

高能天体物理现象 · 物理学 2025-03-06 Hanji Wu , Wei Wang

We present a comprehensive spectral and temporal study of the black hole X-ray transient MAXI J1820+070 during its outbursts in 2018 using Swift/XRT, NICER, NuSTAR and AstroSat observations. The Swift/XRT and NICER spectral study shows a…

高能天体物理现象 · 物理学 2022-04-29 Geethu Prabhakar , Samir Mandal , Athulya M. P , Anuj Nandi

We report the results from the broad-band X-ray monitoring of the new Galactic black hole candidate MAXI J1803$-$298 with the MAXI/GSC and Swift/BAT during its outburst. After the discovery on 2021 May 1, the soft X-ray flux below 10 keV…

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…

高能天体物理现象 · 物理学 2021-10-20 Santanu Mondal , Sandip K. Chakrabarti

Black hole X-ray binaries (BHXRBs) play a crucial role in understanding the accretion of matter onto a black hole. Here, we focus on exploring the transient BHXRB \source~discovered by Swift/BAT and MAXI/GSC during its January 2019…

高能天体物理现象 · 物理学 2023-07-26 Skye R. Heiland , Arka Chatterjee , Samar Safi-Harb , Arghajit Jana , Jeremy Heyl

The rising phase of the 2023-24 outburst of the recently discovered bright transient black hole candidate Swift J1727.8-1613 was monitored by {\it Insight}-HXMT. We study the evolution of hard ($4$-150$ keV) and soft ($2$-$4$ keV) band…

高能天体物理现象 · 物理学 2025-09-23 Dipak Debnath , Hsiang-Kuang Chang , Sujoy Kumar Nath , Lev Titarchuk

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…

高能天体物理现象 · 物理学 2018-11-26 Santanu Mondal , Sandip K Chakrabarti

MAXI J1803-298 is a transient black hole candidate discovered in May of 2021 during an outburst that lasted several months. Multiple X-ray observations reveal recurring "dipping" intervals in several of its light curves, particularly during…

We study accretion flow dynamics of Galactic transient black hole candidate (BHC) H 1743-322 during its 2010 outburst by analyzing spectral data using Two Component (Keplerian and sub-Keplerian) Advective Flow (TCAF) solution, after its…

高能天体物理现象 · 物理学 2015-06-18 Santanu Mondal , Dipak Debnath , Sandip K. Chakrabarti

Black hole low mass X-ray binaries in their hard spectral state are found to display two different correlations between the radio emission from the compact jets and the X-ray emission from the inner accretion flow. Here, we present a large…