S
Santanu Mondal
Researcher at Ben-Gurion University of the Negev
Publications - 58
Citations - 1176
Santanu Mondal is an academic researcher from Ben-Gurion University of the Negev. The author has contributed to research in topics: Accretion (meteorology) & Accretion (astrophysics). The author has an hindex of 20, co-authored 41 publications receiving 1056 citations. Previous affiliations of Santanu Mondal include Indian Institute of Astrophysics & Indian Centre for Space Physics.
Papers
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Implementation of two-component advective flow solution in xspec
TL;DR: In this article, Chakrabarti-Titarchuk solution of two component advective flow (TCAF) was used to fit data of several black hole candidates quite satisfactorily.
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Characterization of GX 339-4 outburst of 2010-11: analysis by XSPEC using two component advective flow model
TL;DR: In this article, 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 were compared.
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Inference on accretion flow dynamics using TCAF solution from the analysis of spectral evolution of H 1743-322 during 2010 outburst
TL;DR: In this article, the authors studied the accretion flow dynamics of BHC H 1743-322 during its 2010 outburst by analyzing spectral data using Two Component (Keplerian and sub-Keplerians) Advective Flow (TCAF) solution, after its inclusion in XSPEC as a local model.
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Accretion flow properties of maxi j1543–564 during 2011 outburst from the tcaf solution
TL;DR: In this article, the authors derived accretion flow properties of the transient black hole candidate (BHC) MAXI J1543-564 using the RXTE data and used the two-component advective flow (TCAF) solution to fit the data of the initial rising phase of outburst (from 2011 May 10 to 15).
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Inference on accretion flow dynamics using tcaf solution from the analysis of spectral evolution of h 1743-322 during the 2010 outburst
TL;DR: In this article, the authors used the two-component advective flow (TCAF; Keplerian and sub-Keplerian) solution after its inclusion in XSPEC as a local model to study accretion flow dynamics of the Galactic transient black hole candidate (BHC) H 1743-322 during its 2010 outburst.