X-ray spectral correlations in a sample of Low-mass black hole X-ray binaries in the hard state
arXiv:2302.13576 · doi:10.3847/1538-4357/acba11
Abstract
The power-law emission and reflection component provide valuable insights into the accretion process around a black hole. In this work, thanks to the broadband spectra coverage of \emph{the Nuclear Spectroscopic Telescope Array}, we study the spectral properties for a sample of low-mass black hole X-ray binaries (BHXRBs). We find that there is a positive correlation between the photon index and the reflection fraction (the ratio of the coronal intensity that illuminates the disk to the coronal intensity that reaches the observer), consistent with previous studies, but except for MAXI J1820+070. It is quite interesting that this source also deviates from the well-known ``V"-shaped correlation between the photon index and the X-ray luminosity log, when it is in the bright hard state. More specifically, the -shaped correlation between and log is observed, as the luminosity decreases by a factor of 3 in a narrow range from to . Furthermore, we discover a strong positive correlation between and the X-ray luminosity for BHXRBs in the hard state, which puts a constraint on the disk-corona coupling and the evolution.
arXiv comment18 pages, 9 figures, 3 tables, Accepted for publication in ApJ
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