48 citations · 109 across the 3 of their papers we have counts for
10 papers
What Powered the Kilonova-Like Emission After GRB 230307A in the Framework of a Neutron Star-White Dwarf Merger?
Xiangyu Ivy Wang, Yun-Wei Yu, Jia Ren +3
The second brightest gamma-ray burst, GRB 230307A (with a duration ~ 40 s), exhibited characteristics indicative of a magnetar engine during the prompt emission phase. Not…
A Channel to Form Fast-spinning Black Hole-Neutron Star Binary Mergers as Multimessenger Sources. II. Accretion-induced Spin-up
Zhen-Han-Tao Wang, Rui-Chong Hu, Ying Qin +7
In this work, we investigate an alternative channel for the formation of fast-spinning black hole-neutron star (BHNS) binaries, in which super-Eddington accretion is expected to oc…
Super-Eddington Accretion as a Possible Scenario to Form GW190425
W. T. Zhang, Z. H. T. Wang, J. -P. Zhu +7
On 2019 April 25, the LIGO/Virgo Scientific Collaboration detected a compact binary coalescence, GW190425. Under the assumption of the binary neutron star (BNS), the total mass of…
Revisiting the Properties of GW190814 and Its Formation History
F. Lyu, L. Yuan, D. H. Wu +9
GW190814 was reported during LIGO's and Virgo's third observing run with the most asymmetric component masses (a black hole and a compac…
Polarization Signature of Companion-Fed Supernovae Arising from BH-NS/BH Progenitor Systems
Xudong Wen, He Gao, Shunke Ai +3
The formation of black hole-neutron star (BH-NS) or BH-BH systems may be accompanied with special supernova (SN) signals, due to the accretion feedback from the companion BH. The a…
A Population Study on the Radio Emission of Fast Blue Optical Transients
Jian-Feng Liu, Liang-Duan Liu, Yun-Wei Yu +1
Despite the fact that the progenitor of fast blue optical transients (FBOTs) is still up for debate, FBOTs are sometimes suggested to originate from the core-collapse of ultra-stri…