The mHz quasi-regular modulations of 4U 1630--47 during its 1998 outburst
Qingchang Zhao, Hongxing Yin, Lian Tao, Zixu Yang, Jinlu Qu, Liang, Zhang, Shu Zhang, Erlin Qiao, Qingcui Bu, Shujie Zhao, Panping Li, Yiming, Huang, Ruican Ma, Ruijing Tang, Pei Jin, Wei Yu, Hexin Liu, Yue Huang, Xiang, Ma, Jingyu Xiao, Xuan Zhang, Kang Zhao

TL;DR
This paper investigates the mHz quasi-regular modulation in the black hole binary 4U 1630--47 during its 1998 outburst, revealing flux dependence, correlations with spectral states, and detailed timing behavior.
Contribution
It provides a detailed analysis of the timing and spectral properties of mHz QRM, identifying distinct behaviors and their relation to spectral states, which advances understanding of accretion processes in black hole binaries.
Findings
QRM frequency is flux dependent and varies with spectral hardness.
Different behaviors of QRM and LFQPOs are classified based on power density spectrum analysis.
QRM rms correlates positively with the power-law flux fraction.
Abstract
We present the results of a detailed timing and spectral analysis of the quasi-regular modulation (QRM) phenomenon in the black hole X-ray binary 4U 1630--47 during its 1998 outburst observed by Rossi X-ray Timing Explore (RXTE). We find that the 50-110 mHz QRM is flux dependent, and the QRM is detected with simultaneous low frequency quasi-periodic oscillations (LFQPOs). According to the behavior of the power density spectrum, we divide the observations into four groups. In the first group, namely behavior A, LFQPOs are detected, but no mHz QRM. The second group, namely behavior B, a QRM with frequency above 88 mHz is detected and the 5 Hz and 7 Hz LFQPOs are almost overlapping. In the third group, namely behavior C, the QRM frequency below 88 mHz is detected and the LFQPOs are significantly separated. In the forth group, namely behavior D, neither…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Mechanics and Biomechanics Studies · High-pressure geophysics and materials
