activity
20172023
most citedThe FAST Galactic Plane Pulsar Snapshot Survey: II. Discovery of 76 Galactic rotating radio transients and their enigma

39 citations · 146 across the 11 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

10 papers · 1 filter

astro-ph.HE2023★ 8 cited

Statistical properties and lensing effect on the repeating fast radio burst FRB 180916.J0158+65

Yu-Bin Wang, Abdusattar Kurban, Xia Zhou +2

FRB 180916.J0158+65 is a well-known repeating fast radio burst with a period () and an active window (). We give out the statistical results of the di…

astro-ph.HE2023★ 8 cited

Dynamics of the clumps partially disrupted from a planet around a neutron star

Abdusattar Kurban, Xia Zhou, Na Wang +3

Tidal disruption events are common in the Universe, which may occur in various compact star systems and could account for many astrophysical phenomena. Depending on the separation…

astro-ph.HE2023★ 39 cited

The FAST Galactic Plane Pulsar Snapshot Survey: II. Discovery of 76 Galactic rotating radio transients and their enigma

D. J. Zhou, J. L. Han, Jun Xu +15

We are carrying out the GPPS survey by using the FAST, the most sensitive systematic pulsar survey in the Galactic plane. In addition to about 500 pulsars already discovered throug…

astro-ph.HE2023★ 2 cited

Atlas of dynamic spectra of fast radio burst FRB 20201124A

Bo-Jun Wang, Heng Xu, Jin-Chen Jiang +64

Fast radio bursts (FRBs) are highly dispersed millisecond-duration radio bursts, of which the physical origin is still not fully understood. FRB 20201124A is one of the most active…

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★ 16 cited

Luminosity distribution of fast radio bursts from CHIME/FRB Catalog 1 by means of the updated Macquart relation

Xiang-Han Cui, Cheng-Min Zhang, Di Li +9

Fast radio bursts (FRBs) are extremely strong radio flares lasting several micro- to milliseconds and come from unidentified objects at cosmological distances, most of which are on…

astro-ph.HE2021★ 9 cited

Statistical tests of young radio pulsars with/without supernova remnants: implying two origins of neutron stars

Xiang-Han Cui, Cheng-Min Zhang, Di Li +11

The properties of the young pulsars and their relations to the supernova remnants (SNRs) have been the interesting topics. At present, 383 SNRs in the Milky Way galaxy have been pu…

astro-ph.HE2021★ 7 cited

Statistical properties of fast radio bursts elucidate their origins: magnetars are favoured over gamma-ray bursts

Xiang-Han Cui, Cheng-Min Zhang, Shuang-Qiang Wang +11

Fast radio bursts (FRBs) are extremely strong radio flares lasting several milliseconds, most of which come from unidentified objects at a cosmological distance. They can be appare…

astro-ph.HE2020★ 29 cited

Fast radio bursts: do repeaters and non-repeaters originate in statistically similar ensembles

Xiang-Han Cui, Cheng-Min Zhang, Shuang-Qiang Wang +9

Fast Radio Bursts (FRBs) are the short, strong radio pulses lasting several milliseconds. They are subsequently identified, for the most part, as emanating from unknown objects at…

astro-ph.HE2018★ 9 cited

The r-mode instability windows of strange stars

Yu-Bin Wang, Xia Zhou, Na Wang +1

With the constraint from gravitational wave emission of a binary merger system (GW170817) and two-solar-mass pulsar observations, we investigate the r-mode instability windows of s…