activity
20072022
most citedConstraints on the Mass Accretion Rate of Neutrino-Cooled Disks in Gamma-Ray Bursts

44 citations · 89 across the 7 of their papers we have counts for

collaborators

14 papers

astro-ph.HE202211 cited

Comparing the Super-Eddington accretion of SMC X-3 and RX J0209.6-7427 with Swift J0243.6+6124

Jiren Liu, Georgios Vasilopoulos, MingYu Ge +4

We study the giant outbursts of SMC X-3 and RX J0209.6-7427 to compare their super-Eddington accretion regime with that of Swift J0243.6+6124. The high double-peak profile of SMC X…

astro-ph.HE2022

Radio pulsations from a neutron star within the gamma-ray binary LS I +61 303

Shan-Shan Weng, Lei Qian, Bo-Jun Wang +9

LS I +61 303 is one of the rare gamma-ray binaries, emitting most of their luminosity in photons with energies beyond 100 MeV. The 26.5 d orbital period is clearly…

astro-ph.HE202219 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…

astro-ph.HE2021

Time-lag between disk and corona radiation leads to hysteresis effect observed in black-hole X-ray binary MAXI J1348-630

Shan-Shan Weng, Zhen-Yi Cai, Shuang-Nan Zhang +4

Accretion is an essential physical process in black-hole X-ray binaries (BHXRBs) and active galactic nuclei. The properties of accretion flows and their radiation were originally c…

astro-ph.HE2019

Evolution of hard X-ray photon index in black-hole X-ray binaries: hints for accretion physics

Hao Liu, AiJun Dong, ShanShan Weng +1

The anti- and positive correlations between X-ray photon index and Eddington-scaled X-ray luminosity were found in decay phase of X-ray binary outbursts and a sample of active gala…

astro-ph.HE2019

NuSTAR and XMM-Newton observations of SXP 59 during its 2017 giant outburst

Shan-Shan Weng, Ming-Yu Ge, Hai-Hui Zhao

The Be X-ray pulsar (BeXRP) SXP 59 underwent a giant outburst in 2017 with a peak X-ray luminosity of erg~s. We report on the X-ray behaviour of SXP 59 wi…