The comptonizing medium of the black hole X-ray binary MAXI J1535-571 through type-C quasi-periodic oscillations. Rawat, D., Méndez, M., Garcı́a, Federico, Altamirano, D., Karpouzas, K., Zhang, L., Alabarta, K., Belloni, T. M., Jain, P., & Bellavita, C. \mnras, 520(1):113-128, March, 2023. doi bibtex @ARTICLE{2023MNRAS.520..113R,
author = {{Rawat}, Divya and {M{\'e}ndez}, Mariano and {Garc{\'\i}a}, Federico and {Altamirano}, Diego and {Karpouzas}, Konstantinos and {Zhang}, Liang and {Alabarta}, Kevin and {Belloni}, Tomaso M. and {Jain}, Pankaj and {Bellavita}, Candela},
title = "{The comptonizing medium of the black hole X-ray binary MAXI J1535-571 through type-C quasi-periodic oscillations}",
journal = {\mnras},
keywords = {accretion, accretion discs, black hole physics, methods: observationa, software: data analysis, X-rays: binaries, X-rays: individual: MAXI J1535-571, Astrophysics - High Energy Astrophysical Phenomena},
year = 2023,
month = mar,
volume = {520},
number = {1},
pages = {113-128},
doi = {10.1093/mnras/stad126},
archivePrefix = {arXiv},
eprint = {2301.04418},
primaryClass = {astro-ph.HE},
adsurl = {https://ui.adsabs.harvard.edu/abs/2023MNRAS.520..113R},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
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