Broad Band X-ray Spectra of Atoll Source 4U 1636-536: NuSTAR and Swift   Results
  In this work we investigate broad band (1-79 keV) spectral nature of the atoll source 4U 1636-536 using the combined Nu-STAR and SWIFT-XRT data. The spectra are complex and have emission components from the disc, boundary-layer and corona. In addition to that a broad iron line is also observed. A relativistic line model assuming Schwarzchild metric fits this feature. The total flux varies from 1.4 $\times$ 10$^{-9}$ to 4.36 $\times$ 10$^{-9}$ $ergs/s/cm^2$. At the highest flux level the source was found in the soft state. In this state the Comptonized component has temperature $kT_e \sim 3$ keV and optical depth $\tau \sim $ 16. We also detect a non-thermal tail with index $\sim$ 2.4, contributing $\sim$ 10 \% of the total flux in the soft state. We also find that the inner disc radius, electron temperature and optical depth vary with the total 0.1-100 keV unabsorbed flux. We discuss the implication of the results in this paper. 
Vivek Kumar Agrawal, Mohammad Hasan
astro-ph.HE