most citedOn the Distance of SGR 1935+2154 Associated with FRB 200428 and Hosted in SNR G57.2+0.8

61 citations · 146 across the 5 of their papers we have counts for

collaborators

9 papers

astro-ph.HE2020

On the Energy Sources of the Most Luminous Supernova ASASSN-15lh

Long Li, Zi-Gao Dai, Shan-Qin Wang +1

In this paper, we investigate the energy-source models for the most luminous supernova ASASSN-15lh. We revisit the ejecta-circumstellar medium (CSM) interaction (CSI) model and the…

astro-ph.HE202061 cited

On the Distance of SGR 1935+2154 Associated with FRB 200428 and Hosted in SNR G57.2+0.8

S. Q. Zhong, Z. G. Dai, H. M. Zhang +1

Owing to the detection of an extremely bright fast radio burst (FRB) 200428 associated with a hard X-ray counterpart from the magnetar soft gamma-ray repeater (SGR) 1935+2154, the…

astro-ph.HE202056 cited

Periodic Fast Radio Bursts as a Probe of Extragalactic Asteroid Belts

Z. G. Dai, S. Q. Zhong

The periodic activity of repeating fast radio burst (FRB) 180916.J0158+65 was recently reported by the CHIME/FRB Collaboration team. 28 bursts from this source not only show a $\si…

astro-ph.HE2020

Magnetars from Neutron Star--White Dwarf Mergers: Application to Fast Radio Bursts

Shu-Qing Zhong, Zi-Gao Dai

It is widely believed that magnetars could be born in core-collapse supernovae (SNe), binary neutron star (BNS) or binary white dwarf (BWD) mergers, or accretion-induced collapse (…

astro-ph.HE2019

Physical Implications of the Sub-threshold GRB GBM-190816 and its Associated Sub-threshold Gravitational Wave Event

Yi-Si Yang, Shu-Qing Zhong, Bin-Bin Zhang +10

The LIGO-Virgo and Fermi collaborations recently reported a possible joint detection of a sub-threshold gravitational wave (GW) event and a sub-threshold gamma-ray burst (GRB), GBM…

astro-ph.HE201910 cited

Gravitational Waves from Newborn Accreting Millisecond Magnetars

Shu-Qing Zhong, Zi-Gao Dai, Xiang-Dong Li

Two accretion columns have been argued to form over the surface of a newborn millisecond magnetar for an extremely high accretion rate $\gtrsim1.8\times10^{-2}M_\odot\ {\rm s^{-1}}…