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20162024
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astro-ph.HE2024

A Hydrodynamical Thermal Irradiated Wind from the Outer Thin Accretion Disk in Low-luminosity Active Galactic Nuclei

Nagendra Kumar

Evidently, low-luminosity active galactic nuclei (LLAGNs) are comprised of an inner advective disk and an outer geometrically thin disk. Wind is inevitable in LLAGNs, mainly interp…

astro-ph.HE2023

Plane Polarization in Comptonization process : a Monte Carlo study

Nagendra Kumar

High energies emissions observed in X-ray binaries (XRBs), active galactic nuclei (AGNs) are linearly polarized. The prominent mechanism for X-ray is the Comptonization process. We…

astro-ph.HE2021

Thermal irradiation induced wind outflow in a geometrically thin accretion disk: A hydrodynamic study

Nagendra Kumar, Banibrata Mukhopadhyay

Many astrophysical sources, e.g., cataclysmic variables, X-ray binaries, active galactic nuclei, exhibit a wind outflow, when they reveal a multicolor blackbody spectrum, hence har…

astro-ph.HE2021

Blazars SED in Conical Plasma Flow : a Monte Carlo study

Nagendra Kumar, Pankaj Kushwaha

Blazars host the most powerful persistent relativistic conical jet -- a highly collimated anisotropic flow of material/plasma. Motivated by this, we explore the blazar's broadband…

astro-ph.HE2018

High energy power-law tail in X-ray binaries and bulk Comptonization due to a outflow from a disk

Nagendra Kumar

We study the high energy power-law tail emission of X-ray binaries (XRBs) by a bulk Comptonization process which usually observe in the very high soft VHS state of blackhole BH XRB…

astro-ph.HE2016

Constraining the size of the Comptonizing medium by modeling the energy dependent time-lags of kHz QPOs of Neutron star system

Nagendra Kumar, Ranjeev Misra

In earlier works, we had shown that the observed soft lags and r.m.s versus energy of the lower kHz QPO of neutron star binaries can be explained in the framework of a thermal Comp…