학술논문
An Insight-HXMT view of the mHz quasi-regular modulation phenomenon in the black hole X-ray binary 4U 1630-47
Document Type
Working Paper
Author
Yang, Zi-Xu; Zhang, Liang; Huang, Yue; Bu, Qingcui; Zhang, Zhen; Liu, He-Xin; Yu, Wei; Wang, Peng-Ju; Zhao, Q. C.; Tao, L.; Qu, Jin-Lu; Zhang, Shu; Zhang, Shuang-Nan; Song, Liming; Lu, Fangjun; Cao, Xuelei; Chen, Li; Cai, Ce; Chang, Zhi; Chen, Tianxian; Chen, Yong; Chen, Yupeng; Chen, Yibao; Cui, Weiwei; Ding, Guoqiang; Du, Yuanyuan; Gao, GuanHua; Gao, He; Ge, Mingyu; Gu, Yudong; Guan, Ju; Guo, Chengcheng; Han, Dawei; Huo, Jia; Jia, Shumei; Jiang, Weichun; Jin, Jing; Kong, Lingda; Li, Bing; Li, Gang; Li, Wei; Li, Xian; Li, Xufang; Li, Zhengwei; Li, Chengkui; Lin, Lin; Liu, Congzhan; Li, Tipei; Li, Xiaobo; Liang, Xiaohua; Liao, Jinyuan; Liu, Hongwei; Liu, Xiaojing; Lu, Xuefeng; Luo, Qi; Luo, Tao; Ma, Binyuan; Ma, Ruican; Ma, Xiang; Meng, Bin; Nang, Yi; Nie, Jianyin; Ou, Ge; Ren, Xiaoqin; Sai, Na; Song, Xinying; Sun, Liang; Tan, Ying; Tuo, Youli; Wang, Chen; Wang, Wenshuai; Wang, Lingjun; Wang, Yusa; Wang, Jieshuang; Wen, Xiangyang; Wu, Bobing; Wu, Baiyang; Wu, Mei; Xiao, Shuo; Xu, Yupeng; Xiong, Shaolin; Yang, Sheng; Yang, Yanji; Yi, Qibin; Yin, Qianqing; You, Yuan; Zhang, Bing; Zhang, Fan; Zhang, Hongmei; Zhang, Juan; Zhang, Wanchang; Zhang, Wei; Zhang, Binbin; Zhang, Peng; Zhang, Yifei; Zhang, Yuanhang; Zhao, Haisheng; Zhao, Xiaofan; Zheng, Shijie; Zhou, Dengke
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Subject
Language
Abstract
Here we report the spectral-timing results of the black hole X-ray binary 4U 1630-47 during its 2021 outburst using observations from the Hard X-ray Modulation Telescope. Type-C quasi-periodic oscillations (QPOs) in 1.6--4.2 Hz and quasi-regular modulation (QRM) near 60 mHz are detected during the outburst. The mHz QRM has a fractional rms of 10%--16% in the 8--35 keV energy band with a Q factor (frequency/width) of 2--4. Benefiting from the broad energy band of hxmt, we study the energy dependence of the 60 mHz QRM in 1--100 keV for the first time. We find that the fractional rms of the mHz QRM increases with photon energy, while the time lags of the mHz QRM are soft and decrease with photon energy. Fast recurrence of the mHz QRM, in a timescale of less than one hour, has been observed during the outburst. During this period, the corresponding energy spectra moderately change when the source transitions from the QRM state to the non-QRM state. The QRM phenomena also shows a dependence with the accretion rate. We suggest that the QRM could be caused by an unknown accretion instability aroused from the corona.