Wavelet analysis of the transient QPOs in MAXI J1535-571 with Insight-HXMT

被引：7

作者：

Chen, X. ^{[1
,2
]}

Wang, W. ^{[1
,2
]}

Tian, P. F. ^{[1
,2
]}

Zhang, P. ^{[1
,2
]}

Liu, Q. ^{[1
,2
]}

Wu, H. J. ^{[1
,2
]}

Sai, N. ^{[1
,2
]}

Huang, Y. ^{[3
]}

Song, L. M. ^{[3
]}

Qu, J. L. ^{[3
]}

Tao, L. ^{[3
]}

Zhang, S. ^{[3
]}

Lu, F. J. ^{[3
]}

Zhang, S. N. ^{[3
]}

机构：

[1] Wuhan Univ, Sch Phys & Technol, Dept Astron, Wuhan 430072, Peoples R China

[2] Wuhan Univ, WHU NAOC Joint Ctr Astron, Wuhan 430072, Peoples R China

[3] Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, Beijing 100049, Peoples R China

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2022年 / 517卷 / 01期

关键词：

black hole physics; Stars: individual: MAXI J1535-571; X-rays: binaries; QUASI-PERIODIC OSCILLATIONS; NEUTRON-STAR; XTE J1550-564; GRS 1915+105; BLACK-HOLES; VARIABILITY; JET; ENERGY; COMPTONIZATION; SPECTRA;

D O I：

10.1093/mnras/stac2710

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Using wavelet analysis and power density spectrum, we investigate two transient quasi-periodic oscillations (QPOs) observed in MAXI J1535-571 observed with Insight-HXMT. The transient QPOs have a centroid frequency of similar to 10 Hz with an FWHM similar to 0.6 Hz, and an rms amplitude similar to 14 per cent. Energy spectra of QPO and non-QPO regimes are also separated and analysed, and the spectra become softer with higher E-cut in the non-QPO regime compared to the QPO regime. Our results suggest that the transient QPOs detected in MJD 58016 and 58017 are still the type-C QPO, and the source remains in its HIMS. The duration of all type-C QPO signals based on wavelet is positively correlated with the mean count rate above similar to 10 keV, implying appearance of QPOs in different time-scales should be coupled with the corona. The transient QPO properties could be related to the jet or flares, perhaps the partial ejection of the corona is responsible for the disappearance of the type-C QPO.

引用

页码：182 / 191

页数：10

共 75 条

[61]

[62] X-ray reverberation around accreting black holes [J].