Low Frequency Quasi-periodic Oscillation in MAXI J1820+070: Revealing distinct Compton and Reflection Contributions
Chenxu Gao, Zhen Yan, Wenfei Yu (Shanghai Astronomical Observatory)

TL;DR
This study analyzes LFQPOs in MAXI J1820+070, revealing that high-energy variability originates from Comptonization, while softer energy variations are mainly due to disk reflection, providing insights into the physical origin of these oscillations.
Contribution
It demonstrates that LFQPO flux variations are driven by Comptonization at high energies and reflection at lower energies, offering a detailed spectral-timing analysis of black hole X-ray binaries.
Findings
LFQPO flux at >100 keV is from Compton component.
LFQPO flux at <30 keV is mainly due to reflection.
Reflection fraction increases with LFQPO amplitude.
Abstract
X-ray low frequency quasi-periodic oscillations (LFQPOs) of black hole X-ray binaries, especially those type-C LFQPOs, are representative timing signals of black hole low/hard state and intermediate state, which has been suspected as to originate due to Lense-Thirring precession of the accretion flow. Here we report an analysis of one of the \emph{Insight}-HXMT observations of the black hole transient MAXI J1820070 taken near the flux peak of its hard spectral state during which strong type-C LFQPOs were detected in all three instruments up to photon energies above 150 keV. We obtained and analyzed the short-timescale X-ray spectra corresponding to high- and low-intensity phases of the observed LFQPO waveform with a spectral model composed of Comptonization and disk reflection components. We found that the normalization of the spectral model is the primary parameter that varied…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Astrophysics and Cosmic Phenomena · Astrophysical Phenomena and Observations
