activity
20172025
most citedMass and Age of Red Giant Branch Stars Observed with LAMOST and \emph{Kepler}

52 citations · 143 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.HE2025★ 3 cited

On Ultra-long Period (53.8 min) Pulsar ASKAP J1935+2148: Coherent Radio Emission Triggered by Local Superstrong Magnetic Reconnection

Zhi-Yao Yang, Cheng-Min Zhang, De-Hua Wang +5

The eight ultra-long period pulsars (ULPPs) in radio bands have been discovered recently, e.g., ASKAP J1935+2148 with a spin period of 53.8\,min, which are much longer than those o…

astro-ph.HE2023

Fast radio bursts generated by coherent curvature radiation from compressed bunches for FRB 20190520B

Xiang-han Cui, Zheng-wu Wang, Cheng-min Zhang +4

The radiation mechanism of fast radio bursts (FRBs) has been extensively studied but still remains elusive. Coherent radiation is identified as a crucial component in the FRB mecha…

astro-ph.HE2022★ 4 cited

Distribution of fast radio burst dispersion measures in CHIME/FRB Catalog 1: implications on the origin of FRBs

Jianwei Zhang, Chengmin Zhang, Di Li +7

Recently, CHIME/FRB project published its first fast radio burst (FRB) catalog (hereafter, Catalog 1), which totally contains 536 unique bursts. With the help of the latest set of…

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★ 5 cited

Simulation of the orbit and spin period evolution of the double pulsars PSR J0737-3039 from their birth to coalescence induced by the gravitational wave radiation

Peng Liu, Yi-Yan Yang, Jian-Wei Zhang +1

The complete orbital and sin period evolutions of the double neutron star (NS) system PSR J0737-3039 are simulated from the birth to coalescence, which include the two observed rad…

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.SR2017★ 52 cited

Mass and Age of Red Giant Branch Stars Observed with LAMOST and \emph{Kepler}

Yaqian Wu, Maosheng Xiang, Shaolan Bi +13

Obtaining accurate and precise masses and ages for large numbers of giant stars is of great importance for unraveling the assemblage history of the Galaxy. In this paper, we estima…