We study the spectral properties of Galactic transient black hole candidate H 1743-322 during its early phase of 2010 outburst with Two Component Advective Flow (TCAF) model, after its inclusion in spectral analysis software package XSPEC as a local model. For the analysis, spectral data from RXTE/PCA instrument in 2.5-25 keV energy band are used. From the spectral fit, accretion flow parameters such as Keplerian (disk) rate, sub-Keplerian (halo) rate, location of the shock and strength of the shock are directly extracted. QPO frequencies are predicted from the TCAF model spectral fitted shock parameters, `closely' matches with the observed frequencies.
@article{arxiv.1309.3604,
title = {Extracting Flow parameters of H 1743-322 during early phase of its 2010 outburst using Two Component Advective Flow model},
author = {Dipak Debnath and Sandip K. Chakrabarti and Santanu Mondal},
journal= {arXiv preprint arXiv:1309.3604},
year = {2013}
}