A Phase-resolved View of the Low-frequency Quasiperiodic Oscillations from the Black Hole Binary MAXI J1820+070

• Published in: The Astrophysical journal Vol. 957; no. 2; pp. 84 - 98
• Main Authors: Shui, Qing C., Zhang, S., Zhang, Shuang N., Chen, Yu P., Kong, Ling D., Wang, Peng J., Peng, Jing Q., Ji, L., Santangelo, A., Yin, Hong X., Qu, Jin L., Tao, L., Ge, Ming Y., Huang, Y., Zhang, L., Liu, Hong H., Zhang, P., Yu, W., Chang, Z., Li, J., Ye, Wen T., Li, Pan P., Yu, Zhuo L., Yan, Z.
• Format: Journal Article
• Language: English
• Published: Philadelphia The American Astronomical Society 01.11.2023; IOP Publishing
• Subjects: Accretion; Astrophysics; Black holes; Corona; Data points; Deposition; Energy bands; Harmonics; Light curve; Oscillations; Outbursts; Resonant frequencies; Spectral analysis; Spectroscopy; Spectrum analysis; Stellar mass black holes; Waveforms; X ray binaries; X ray stars; X-ray astronomy; X-ray binary stars
• ISSN: 0004-637X; 1538-4357
• DOI: 10.3847/1538-4357/acfc42

Abstract Although low-frequency quasiperiodic oscillations (LFQPOs) are commonly detected in the X-ray light curves of accreting black hole X-ray binaries, their origin still remains elusive. In this study, we conduct phase-resolved spectroscopy in a broad energy band for LFQPOs in MAXI J1820+070 during its 2018 outburst, utilizing Insight-HXMT observations. By employing the Hilbert–Huang transform method, we extract the intrinsic quasiperiodic oscillation (QPO) variability, and obtain the corresponding instantaneous amplitude, phase, and frequency functions for each data point. With well-defined phases, we construct QPO waveforms and phase-resolved spectra. By comparing the phase-folded waveform with that obtained from the Fourier method, we find that phase folding on the phase of the QPO fundamental frequency leads to a slight reduction in the contribution of the harmonic component. This suggests that the phase difference between QPO harmonics exhibits time variability. Phase-resolved spectral analysis reveals strong concurrent modulations of the spectral index and flux across the bright hard state. The modulation of the spectral index could potentially be explained by both the corona and jet precession models, with the latter requiring efficient acceleration within the jet. Furthermore, significant modulations in the reflection fraction are detected exclusively during the later stages of the bright hard state. These findings provide support for the geometric origin of LFQPOs and offer valuable insights into the evolution of the accretion geometry during the outburst in MAXI J1820+070.