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Testing Comptonization as the Origin of the Continuum in Nonmagnetic Cataclysmic Variables: The Photon Index of X-Ray Emission
T. Maiolino, L. Titarchuk, F. D’Amico, Z. Q. Cheng, W. Wang, M. Orlandini and Filippo Frontera The Astrophysical Journal 900(2) 153 (2020) https://doi.org/10.3847/1538-4357/abab93
Timing Properties of Shocked Accretion Flows around Neutron Stars in the Presence of Cooling
Exploring the Universe: From Near Space to Extra-Galactic
Ayan Bhattacharjee Astrophysics and Space Science Proceedings, Exploring the Universe: From Near Space to Extra-Galactic 53 93 (2018) https://doi.org/10.1007/978-3-319-94607-8_8
Effect of non-stationary accretion on spectral state transitions: An example of a persistent neutron star LMXB 4U1636–536
Monte Carlo simulations of thermal comptonization process in a two-component advective flow around a neutron star
Ayan Bhattacharjee and Sandip K. Chakrabarti Monthly Notices of the Royal Astronomical Society 472(2) 1361 (2017) https://doi.org/10.1093/mnras/stx1867
X-RAY SPECTRA OF THE HIGH-MASS X-RAY BINARY 4U 1700-37 USING BEPPOSAX, SUZAKU, AND RXTE OBSERVATIONS
Iron-line and continuum variations in the XMM–Newton and Suzaku spectra of the neutron-star low-mass X-ray binary 4U 1636−53
Ming Lyu, Mariano Méndez, Andrea Sanna, et al. Monthly Notices of the Royal Astronomical Society 440(2) 1165 (2014) https://doi.org/10.1093/mnras/stu279
X-RAY SPECTRAL AND TIMING BEHAVIOR OF SCORPIUS X-1. SPECTRAL HARDENING DURING THE FLARING BRANCH