Jet properties of XTE J1752−223 during its 2009–2010 outburst

Galactic short orbital period black hole candidate (BHC) XTE~J1752-223 was discovered on 2009 Oct 21 by the Rossi X-ray Timing Explorer (RXTE). We study spectral properties of this outburst using transonic flow solution based two component advective (TCAF) model. TCAF model fitted spectrum gives an estimation physical parameters, such as Keplerian disk rate, sub-Keplerian halo so-called {\it{Compton cloud}}, other than mass source and normalization ($N$). $N$ is a standardized ratio emitted to observed photon flux in which does not include emission from jets. In presence jets, changes deviation used obtain contribution Nature jet found be compact during low luminous hard state discrete or blobby high intermediate states. find correlation between radio (5.5 GHz) ($2.5-25$ keV) fluxes different components. The ($F_R$) ($F_{ouf}$) are correlated within acceptable range standard ($0.6$ $0.7$). A similar indices were reported our group for three transient BHCs (Swift~J1753.5-0127, MAXI~J1836-194 \& XTE~J1118+480).