Timing analysis of Swift J1658.2-4242's outburst in 2018 with Insight-HXMT, NICER and AstroSat

被引：15
|
作者：
Xiao, G. C. [1 ,2 ]
Lu, Yu [1 ]
Ma, X. [1 ]
Ge, M. Y. [1 ]
Yan, L. L. [3 ]
Li, Z. J. [4 ]
Tuo, Y. L. [1 ,2 ]
Zhang, Y. [1 ,2 ]
Zhang, W. [1 ,2 ]
Liu, H. X. [1 ,2 ]
Zhou, D. K. [1 ,2 ]
Zhang, L. [1 ]
Bu, Q. C. [1 ]
Cao, X. L. [1 ]
Jiang, W. C. [1 ]
Chen, Y. P. [1 ]
Zhang, S. [1 ,2 ]
Lu, F. J. [1 ,2 ]
Chen, L. [5 ]
Qu, J. L. [1 ,2 ]
Song, L. M. [1 ,2 ]
Zhang, S. N. [1 ,2 ]
Zhuang, R. L. [6 ]
Shang, R. C. [7 ]
Jin, Y. J. [6 ]
机构：
[1] Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, Beijing 100049, Peoples R China
[2] Univ Chinese Acad Sci, Beijing 100049, Peoples R China
[3] Anhui Jianzhu Univ, Sch Math & Phys, Hefei 230601, Anhui, Peoples R China
[4] Hebei Univ Engn, Sch Architecture & Art, Handan 056038, Peoples R China
[5] Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China
[6] Tsinghua Univ, Dept Engn Phys, Beijing 100084, Peoples R China
[7] Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China
来源：
JOURNAL OF HIGH ENERGY ASTROPHYSICS | 2019年 / 24卷
基金：
中国国家自然科学基金;
关键词：
Accretion; accretion disks; Black hole physics; X-rays: binaries: Swift J1658.2-4242; QUASI-PERIODIC OSCILLATIONS; X-RAY-PROPERTIES; PHASE LAGS; CENTROID FREQUENCY; ENERGY-DEPENDENCE; GX; 339-4; VARIABILITY; EVOLUTION; EMISSION; EJECTION;
D O I：
10.1016/j.jheap.2019.09.005
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present the observational results from a detailed timing analysis of the black hole candidate Swift J1658.2-4242 during its 2018 outburst with the observations of Hard X-ray Modulation Telescope (Insight-HXMT), Neutron Star Interior Composition Explorer (NICER) and AstroSat in 0.1-250 keV. The evolution of intensity, hardness and integrated fractional root mean square (rms) observed by Insight-HXMT and NICER are presented in this paper. Type-C quasi-periodic oscillations (QPOs) observed by NICER (0.8-3.5Hz) and Insight-HXMT (1-1.6Hz) are also reported in this work. The features of the QPOs are analyzed with an energy range of 0.5-50 keV. The relations between QPO frequency and other characteristics such as intensity, hardness and QPO rms are carefully studied. The timing and spectral properties indicate that Swift J1658.2-4242 is a black hole binary system. Besides, the rms spectra of the source calculated from the simultaneous observation of Insight-HXMT, NICER and AstroSat support the LenseThirring origin of the QPOs. The relation between QPO phase lag and the centroid frequency of Swift J1658.2-4242 reveals a near zero constant when < 4Hz and a soft phase lag at 6.68Hz. This independence follows the same trend as the high inclination galactic black hole binaries such as MAXI J1659-152. (C) 2019 Elsevier B.V. All rights reserved.
引用
收藏
页码：30 / 40
页数：11
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