Qingwen Tang
0000-0001-7471-8451
Nanchang University
3 papers found
Refreshing results…
A Channel to Form Fast-spinning Black Hole–Neutron Star Binary Mergers as Multimessenger Sources. II. Accretion-induced Spin-up
Super-Eddington accretion as a possible scenario to form GW190425
Revisiting the properties of GW190814 and its formation history
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