Analysis of NuSTAR and Suzaku observations of Cyg X-1 in the hard state: evidence for a truncated disc geometry. Basak, R., Zdziarski, A. A., Parker, M., & Islam, N. \mnras, 472(4):4220-4232, December, 2017. doi bibtex @ARTICLE{2017MNRAS.472.4220B,
author = {{Basak}, Rupal and {Zdziarski}, Andrzej A. and {Parker}, Michael and {Islam}, Nazma},
title = "{Analysis of NuSTAR and Suzaku observations of Cyg X-1 in the hard state: evidence for a truncated disc geometry}",
journal = {\mnras},
keywords = {accretion, accretion discs, black hole physics, stars: individual: Cyg X-1, X-rays: binaries, X-rays: individual: Cyg X-1, stars: individual: Cyg X-1 - X-rays: binaries, Astrophysics - High Energy Astrophysical Phenomena},
year = 2017,
month = dec,
volume = {472},
number = {4},
pages = {4220-4232},
doi = {10.1093/mnras/stx2283},
archivePrefix = {arXiv},
eprint = {1705.06638},
primaryClass = {astro-ph.HE},
adsurl = {https://ui.adsabs.harvard.edu/abs/2017MNRAS.472.4220B},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
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