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Implementation of two-component advective flow solution in xspec
Spectral and temporal properties of black hole candidates can be explained reasonably well
using Chakrabarti–Titarchuk solution of two-component advective flow (TCAF). This model …
using Chakrabarti–Titarchuk solution of two-component advective flow (TCAF). This model …
Estimation of mass of compact object in H 1743-322 from 2010 and 2011 outbursts using TCAF solution and spectral index–QPO frequency correlation
The well-known black hole candidate (BHC) H 1743-322 exhibited temporal and spectral
variabilities during several outbursts. The variation of the accretion rates and flow geometry …
variabilities during several outbursts. The variation of the accretion rates and flow geometry …
Accretion flow dynamics of MAXI J1836-194 during its 2011 outburst from TCAF solution
The Galactic transient X-ray binary MAXI J1836-194 was discovered on 2011 August 29.
Here we make a detailed study of the spectral and timing properties of its 2011 outburst …
Here we make a detailed study of the spectral and timing properties of its 2011 outburst …
Inference on accretion flow dynamics using TCAF solution from the analysis of spectral evolution of H 1743-322 during the 2010 outburst
We study accretion flow dynamics of the Galactic transient black hole candidate (BHC) H
1743-322 during its 2010 outburst by analyzing spectral data using the two-component …
1743-322 during its 2010 outburst by analyzing spectral data using the two-component …
Estimation of the mass of the black hole candidate MAXI J1659− 152 using TCAF and POS models
The Galactic transient black hole candidate (BHC) MAXI J1659− 152 exhibited temporal and
spectral evolution during its very first X-ray outburst (2010) after its discovery on 2010 …
spectral evolution during its very first X-ray outburst (2010) after its discovery on 2010 …
Characterization of GX 339-4 outburst of 2010–11: analysis by xspec using two component advective flow model
We study spectral properties of GX 339-4 during its 2010–11 outburst with two component
advective flow (TCAF) model after its inclusion in xspec as a table model. We compare …
advective flow (TCAF) model after its inclusion in xspec as a table model. We compare …
Accretion Flow Evolution of a New Black Hole Candidate MAXI J1348–630 during the 2019 Outburst
Galactic black hole (BH) candidate MAXI J1348–630 was recently discovered by MAXI and
Swift/BAT satellites during its first outburst in 2019 January, which continued for∼ 4 months …
Swift/BAT satellites during its first outburst in 2019 January, which continued for∼ 4 months …
Accretion flow properties of MAXI J1543–564 during 2011 outburst from the TCAF solution
We derive accretion flow properties of the transient black hole candidate (BHC) MAXI J1543–
564 using the RXTE data. We use the two-component advective flow (TCAF) solution to fit …
564 using the RXTE data. We use the two-component advective flow (TCAF) solution to fit …
Accretion flow dynamics of MAXI J1659-152 from the spectral evolution study of its 2010 outburst using the TCAF solution
Transient black hole candidates are interesting objects to study in X-rays as these sources
show rapid evolutions in their spectral and temporal properties. In this paper, we study the …
show rapid evolutions in their spectral and temporal properties. In this paper, we study the …
Smoothed particle hydrodynamic simulations of viscous accretion discs around black holes
G Lanzafame, D Molteni… - Monthly Notices of the …, 1998 - academic.oup.com
Viscous Keplerian discs become sub-Keplerian close to a black hole since they pass
through sonic points before entering into it. We study the time evolution of polytropic viscous …
through sonic points before entering into it. We study the time evolution of polytropic viscous …