output
19972026
most citedUltrasensitive and broadband MoS2 photodetector driven by ferroelectrics

856 citations

Showing 2022 · astro-ph.HEShow all

19 papers · 2 filters

astro-ph.HE2022★ 18 cited

Evolution of Spin Period and Magnetic Field of the Crab Pulsar: Decay of the Braking Index by the Particle Wind Flow Torque

Cheng-Min Zhang, Xiang-Han Cui, Di Li +8

The evolutions of a neutron star's rotation and magnetic field (B-field) have remained unsolved puzzles for over half a century. We ascribe the rotational braking torques of pulsar…

astro-ph.HE2022★ 15 cited

Type I X-ray bursts' spectra and fuel composition from the atoll and transient source 4U 173022

Yongqi Lu, Zhaosheng Li, Yuanyue Pan +8

NICER observed two outbursts from the neutron star low-mass X-ray binary 4U~173022 in 2021 and 2022, which showed a similar spectral evolution in the hardness-intensity diagram.…

astro-ph.HE2022★ 3 cited

Studying the properties of compressible MHD turbulence by synchrotron fluctuation statistics

Ru-Yue Wang, Jian-Fu Zhang, Alex Lazarian +2

We study the observable properties of compressible MHD turbulence covering different turbulence regimes, based on synthetic synchrotron observations arising from 3D MHD numerical s…

astro-ph.HE2022★ 4 cited

Return of 4U~1730--22 after 49 years silence: the peculiar burst properties of the 2021/2022 outbursts observed by Insight-HXMT

Yu-Peng Chen, Shu Zhang, Long Ji +10

After in quiescence for 49 years, 4U~1730--22 became active and had two outbursts in 2021 \& 2022; ten thermonuclear X-ray bursts were detected with Insight-HXMT. Among them, the f…

astro-ph.HE2022★ 10 cited

An Insight-HXMT view of the mHz quasi-regular modulation phenomenon in the black hole X-ray binary 4U 1630-47

Zi-Xu Yang, Liang Zhang, Yue Huang +97

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 qu…

astro-ph.HE2022★ 69 cited

Insight-HXMT discovery of the highest energy CRSF from the first Galactic ultra-luminous X-ray pulsar Swift J0243.6+6124

Ling-Da Kong, Shu Zhang, Shuang-Nan Zhang +15

The detection of cyclotron resonance scattering features (CRSFs) is the only way to directly and reliably measure the magnetic field near the surface of a neutron star (NS). The br…

astro-ph.HE2022★ 11 cited

Study on the magnetic field strength of NGC 300 ULX1

Y. Y. Pan, Z. S. Li, C. M. Zhang +1

NGC 300 ULX1 is a pulsating ultraluminous X-ray source (PULX) with the longest spin period of and a high spin-up rate of $\dot P\simeq5.56\times10^{-7}\,\rm s\…

astro-ph.HE2022★ 13 cited

Discovery of a 584.65 Hz Burst Oscillation in the Low Mass X-Ray Binary 4U 1730--22

Zhaosheng Li, Wenhui Yu, Yongqi Lu +2

Type-I X-ray burst oscillations are powered by thermonuclear released on the neutron star (NS) surface in low mass X-ray binaries (LMXBs), where the burst oscillation frequencies a…

astro-ph.HE2022★ 26 cited

Revisit the periodicity of SGR J1935+2154 bursts with updated sample

Sheng-Lun Xie, Ce Cai, Shao-Lin Xiong +30

Since FRB 200428 has been found to be associated with an X-ray burst from the Galactic magnetar SGR J1935+2154, it is interesting to explore whether the magnetar bursts also follow…

astro-ph.HE2022★ 36 cited

The Peculiar Precursor of a Gamma-Ray Burst from a Binary Merger Involving a Magnetar

Shuo Xiao, Yan-Qiu Zhang, Zi-Pei Zhu +42

The milestone discovery of GW 170817-GRB 170817A-AT 2017gfo has shown that gravitational wave (GW) could be produced during the merger of neutron star-neutron star/black hole and t…

astro-ph.HE2022★ 4 cited

The origin of UV/optical emission in the black hole low-mass X-ray binary Swift J1753.5-0127

Pengcheng Yang, Guobao Zhang, David M. Russell +4

The emission from the accreting black holes (BHs) in low-mass X-ray binaries (LMXBs) covers a broad energy band from radio to X-rays. Studying the correlations between emission in…

astro-ph.HE2022★ 24 cited

Insight-HXMT dedicated 33-day observation of SGR J1935+2154 II. Burst Spectral Catalog

Ce Cai, Shaolin Xiong, Lin Lin +21

Since April 28, 2020, Insight-HXMT has implemented a dedicated observation on the magnetar SGR J1935+2154. Thanks to the wide energy band (1-250 keV) and high sensitivity of Insigh…

astro-ph.HE2022★ 3 cited

A Study on the X-Ray Pulse Profile and Spectrum of the Crab Pulsar Using NICER and Insight-HXMT's Observations

Lin-Li Yan, You-Li Tuo, Ming-Yu Ge +3

We analyze the energy dependence of the X-ray pulse profile and the phase-resolved spectra (PRS) of the Crab pulsar using observations from the Neutron star Interior Composition Ex…

astro-ph.HE2022★ 46 cited

Quasi-periodic oscillations of the X-ray burst from the magnetar SGR J1935+2154 and associated with the fast radio burst FRB 200428

Xiaobo Li, Mingyu Ge, Lin Lin +92

The origin(s) and mechanism(s) of fast radio bursts (FRBs), which are short radio pulses from cosmological distances, have remained a major puzzle since their discovery. We report…

astro-ph.HE2022★ 36 cited

Insight-HXMT dedicated 33-day observation of SGR J1935+2154 I. Burst Catalog

Ce Cai, Wangchen Xue, Chengkui Li +21

Magnetars are neutron stars with extreme magnetic field and sometimes manifest as soft gamma-ray repeaters (SGRs). SGR J1935+2154 is one of the most prolific bursters and the first…

astro-ph.HE2022★ 22 cited

The First Insight-HXMT Gamma-Ray Burst Catalog: The First Four Years

Xin-Ying Song, Shao-Lin Xiong, Shuang-Nan Zhang +40

The Hard X-ray Modulation Telescope (Insight-HXMT), is China's first X-ray astronomy satellite launched on June 15, 2017. The anti-coincidence CsI detectors of the High Energy X-ra…

astro-ph.HE2022★ 1 cited

Measurement of MHD turbulence properties by synchrotron radiation techniques

Jianfu Zhang, Ruyue Wang

It is well-known that magnetohydrodynamic (MHD) turbulence is ubiquitous in astrophysical environments. The correct understanding of the fundamental properties of MHD turbulence is…

astro-ph.HE2022★ 20 cited

NICER observations of the evidence of Poynting-Robertson drag and disk reflection during type I X-ray bursts from 4U 1636536

Guoying Zhao, Zhaosheng Li, Yuanyue Pan +4

Type I X-ray bursts are the result of an unstable thermonuclear burning of accreting matter on the neutron star (NS) surface. The quick release of energetic X-ray photons during su…

astro-ph.HE2022★ 19 cited

Peculiar disk behaviors of the black hole candidate MAXI J1348-630 in the hard state observed by Insight-HXMT and Swift

W. Zhang, L. Tao, R. Soria +93

We present a spectral study of the black hole candidate MAXI J1348-630 during its 2019 outburst, based on monitoring observations with Insight-HXMT and Swift. Throughout the outbur…