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Cited article:

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Timing Properties of Shocked Accretion Flows around Neutron Stars in the Presence of Cooling

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Effect of non-stationary accretion on spectral state transitions: An example of a persistent neutron star LMXB 4U1636–536

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Electron–Positron Pair Creation Close to a Black Hole Horizon: Redshifted Annihilation Line in the Emergent X-Ray Spectra of a Black Hole. I.

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Monte Carlo simulations of thermal comptonization process in a two-component advective flow around a neutron star

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Warm and optically thick dissipative coronae above accretion disks

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Iron-line and continuum variations in the XMM–Newton and Suzaku spectra of the neutron-star low-mass X-ray binary 4U 1636−53

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X-RAY SPECTRAL AND TIMING BEHAVIOR OF SCORPIUS X-1. SPECTRAL HARDENING DURING THE FLARING BRANCH

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BLACK HOLE MASS DETERMINATION IN THE X-RAY BINARY 4U 1630-47: SCALING OF SPECTRAL AND VARIABILITY CHARACTERISTICS

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SPECTRAL STATE EVOLUTION OF 4U 1820–30: THE STABILITY OF THE SPECTRAL INDEX OF THE COMPTONIZATION TAIL

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Numerical solution of the radiative transfer equation: X-ray spectral formation from cylindrical accretion onto a magnetized neutron star

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