6 citations · 13 across the 10 of their papers we have counts for
10 papers
Formation of millisecond pulsar-helium star binaries
Zhu-Ling Deng, Xiang-Dong Li, Yong Shao +2
PSR J1928+1815, the first recycled pulsar-helium (He) star binary discovered by the Five-hundred-meter Aperture Spherical radio Telescope, consists of a 10.55 ms pulsar and a compa…
Formation of a Possible Black-hole Ultracompact X-ray Binary with the Shortest Orbital Period
Xing-Peng Yang, Kun Xu, Zhi-Fu Gao +2
In the bulge of M31, the Chandra observations discovered a possible black hole (BH) ultracompact X-ray binary (UCXB) Seq.1 with an orbital period of 7.7 minutes and a maximum X-ray…
On the Formation of the Double Neutron Star Binary PSR J1846-0513
Long Jiang, Kun Xu, Shuai Zha +5
The double neutron star PSR J1846-0513 is discovered by the Five-hundred-meter Aperture Spherical radio Telescope (FAST) in Commensal Radio Astronomy FAST Survey. The pulsar is rev…
On the Interacting/Active Lifetime of Supernova Fallback Disk around Isolated Neutron Stars
Kun Xu, Hao-Ran Yang, Long Jiang +3
The fallback disk model is widely accepted to explain long-period neutron stars (NSs) which can't be simulated by magnetic dipole radiation. However, no confirmed detection of disk…
Formation of PSR J1012+5307 with an extremely low-mass white dwarf: testing magnetic braking models
Na Wei, Kun Xu, Zhi-Fu Gao +2
PSR J1012+5307 is a millisecond pulsar with an extremely low-mass (ELM) white dwarf (WD) companion in an orbit of 14.5 hours. Magnetic braking (MB) plays an important role in influ…
Electron-capture supernovae in NS+He star systems and the double neutron star systems
Yun-Lang Guo, Bo Wang, Wen-Cong Chen +4
Electron-capture supernovae (EC-SNe) provide an alternative channel for producing neutron stars (NSs). They play an important role in the formation of double NS (DNS) systems and t…
Black Hole Ultracompact X-Ray Binaries as Galactic Low-frequency Gravitational Wave Sources: the He Star Channel
Ke Qin, Kun Xu, Dong-Dong Liu +3
Black hole (BH) ultracompact X-ray binaries (UCXBs) are potential Galactic low-frequency gravitational wave (GW) sources. As an alternative channel, BH UCXBs can evolve from BH+He…
Anomalous orbital expansion of low-mass X-ray binary 2A 1822-371: the existence of a circumbinary disk?
Na Wei, Long Jiang, Wen-Cong Chen
The source 2A 1822-371 is an eclipsing low-mass X-ray binary (LMXB) consisting of a neutron star (NS) and a donor star in an orbit of 5.57 hr. Based on timing o…
White Dwarf Mass Growth in Cataclysmic Variables: Roles of Dwarf Novae
Wei-Min Liu, Long Jiang, Wen-Cong Chen +1
The disc instability mechanism (DIM) is widely accepted to account for the transient behaviour of dwarf novae (DNe), which experience short outbursts separated by long quiescence.…
Type Ia supernovae in NS+He star systems and the isolated mildly recycled pulsars
Yun-Lang Guo, Bo Wang, Cheng-Yuan Wu +3
Type Ia supernovae (SNe Ia) are successful cosmological distance indicators and important element factories in the chemical evolution of galaxies. They are generally thought to ori…