24 citations · 101 across the 10 of their papers we have counts for
10 papers
Optical Properties of Crich (C, SiC and FeC) Dust Layered Structure of Massive Stars
Ruiqing Wu, Mengqiu Long, Xiaojiao Zhang +9
The composition and structure of interstellar dust are important and complex for the study of the evolution of stars and the \textbf{interstellar medium} (ISM). However, there is a…
Post-merger evolution of double helium white dwarfs and distribution of helium-rich hot subdwarfs
Jinlong Yu, Xianfei Zhang, Guoliang Lv
The mergers of double helium white dwarfs are believed to form isolated helium-rich hot subdwarfs. Observation shows that the helium-rich hot subdwarfs can be divided into two subg…
Quiescent luminosities of accreting neutron stars with different equation of states
Helei Liu, Akira Dohi, Masa-aki Hashimoto +3
We model the quiescent luminosity of accreting neutron stars with several equation of states (EOSs), including the effect of pion condensation and superfluidity. As a consequence o…
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…
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).…
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…