activity
20182020
most citedPossible Formation Scenarios of ZTF J153932.16+502738.8-A Gravitational Source Close to the Peak of LISA's Sensitivity

16 citations · 35 across the 4 of their papers we have counts for

collaborators

7 papers

astro-ph.SR202016 cited

Possible Formation Scenarios of ZTF J153932.16+502738.8-A Gravitational Source Close to the Peak of LISA's Sensitivity

Guoliang Lü, Chunhua Zhu, Zhaojun Wang +4

ZTF J153932.16+502738.8 (ZTFJ1539) is an eclipsing double-white-dwarf system with an orbital period of 6.91 minutes, and is a significant source of LISA detecting gravitational wav…

astro-ph.SR20196 cited

The Formation of Bimodal Dust Species in Nova Ejecta

Adili Duolikun, Chunhua Zhu, Zhaojun Wang +4

The formation of bimodal dust species (namely the silicate and amorphous carbon dust grains coexistent) in a nova eruption is an open problem. According to the nova model simulated…

astro-ph.HE2019

Quark Novae: An Alternative Channel For the Formation of Isolated Millisecond Pulsars

Nurimangul Nurmamat, Chunhua Zhu, Guoliang Lü +3

Isolated millisecond pulsars (IMSPs) are a topic of academic contention. There are various models to explain their formation. We explore the formation of IMSP via quark novae (QN).…

astro-ph.SR201910 cited

The Formation of Bimodal Dust Species in Nova Ejecta I: Chemical Conditions

Chunhua Zhu, Helei Liu, Guoliang Lü +2

The formation of bimodal dust species (that is, both of silicate and amorphous carbon dust grains are observed in a nova eruption) in nova ejecta is still debated. Using the Module…

astro-ph.HE20183 cited

On Isolated Millisecond Pulsars Formed by the Coalescence of Neutron Stars and Massive White Dwarfs

Shengnan Sun, Lin Li, Helei Liu +3

This paper uses population synthesis to investigate the possible origin of isolated millisecond pulsars (IMSPs) as born from the coalescence of a neutron star (NS) and a white dwar…

astro-ph.HE2018

Magnetic-oscillation mechanism for understanding periodic or quasi-periodic modulation of the timing residuals from pulsars

Zhaojun Wang, Guoliang Lü, Chunhua Zhu +2

Highly precise pulsar timing is very important for understanding the nature of neutron stars and the implied physics, even being used to detect directly gravitational waves. Unfort…