10 citations · 21 across the 14 of their papers we have counts for
14 papers
The Influence of Evaporation on the Formation and Evolution of Huntsman Systems
Hao-Ran Yang, Shi-Jie Gao, Xiang-Dong Li +2
Huntsman systems are a recently identified and rare subclass of millisecond pulsar (MSP) binaries, characterized by a detached neutron star and an evolved giant companion in relati…
Formation of Recycled Pulsars in Common Envelope Binaries
Yu-Dong Nie, Yong Shao, Jian-Guo He +4
We present a systematic study of the evolution of low- and intermediate-mass X-ray binaries (L/IMXBs) consisting of a neutron star (NS) and a donor star of mass $1…
Pulsar Gleaners: Discovery of 19 Pulsars in FAST Archival Data at and Decl.
Shi-Jie Gao, Yi-Xuan Shao, Xiang-Dong Li
We report the discovery of 19 new pulsars identified from archival observations of the Five-hundred-meter Aperture Spherical radio Telescope (FAST) within Galactic latitudes $|b|<5…
Search for Radio Pulsations from Neutron Star Candidates in Detached Binaries
Shi-Jie Gao, Xiang-Dong Li, Song Wang +7
Recent optical astrometric and spectroscopic surveys have identified numerous neutron star (NS) candidates in non-accreting detached binary systems, but their compact-object nature…
Polar Mounds on Strangeon Stars: the Neutrino Emission from Ultraluminous X-ray Pulsars
Hong-Bo Li, Shi-Jie Gao, Xiang-Dong Li +1
Ultraluminous X-ray pulsars (ULXPs) serve as unique astrophysical laboratories, offering critical insights into accretion physics under extreme conditions, such as strong magnetic…
RRAT J2325-0530: A Rotating Radio Transient with an Atypical Waiting-time Distribution
Shi-Jie Gao, Xiang-Dong Li, Zhen Yan +2
We present 1.25 GHz observations of the rotating radio transient (RRAT) J2325-0530, conducted with the Five-hundred-meter Aperture Spherical radio Telescope (FAST). Approximately 6…
A Target Search for Fast Radio Bursts Associated with Two Fast Blue Optical Transients: AT2018cow and CSS161010
Shi-Jie Gao, Xiang-Dong Li, Yi-Xuan Shao +5
Fast blue optical transients (FBOTs) are luminous, rapidly evolving events with blue spectra, possibly powered by newborn magnetars and linked to fast radio bursts (FRBs). Given th…
A Be star-black hole binary with a wide orbit from LAMOST time-domain survey
Qian-Yu An, Yang Huang, Wei-Min Gu +21
Binary systems consisting of an early type star and a black hole (BH) are crucial for understanding various astrophysical phenomena, particularly the origins of detected gravitatio…
Instability in supernova fallback disks and its effect on the formation of ultra long period pulsars
Hao-Ran Yang, Xiang-Dong Li, Shi-Jie Gao +1
Several pulsars with unusually long periods were discovered recently, comprising a potential population of ultra long period pulsars (ULPPs). The origin of their long periodicity i…
Discovery of a millisecond pulsar associated with Terzan 6
Shi-Jie Gao, Yi-Xuan Shao, Pei Wang +6
Observations show that globular clusters might be among the best places to find millisecond pulsars. However, the globular cluster Terzan 6 seems to be an exception without any pul…
The White Dwarf Mass-Orbital Period Relation Under Wind Mass Loss
Shi-Jie Gao, Xiang-Dong Li
Helium white dwarfs (HeWDs) are thought to form from low-mass red giant stars experiencing binary interaction. Because the helium core mass of a red giant star is closely related t…
Can cosmologically-coupled mass growth of black holes solve the mass gap problem?
Shi-Jie Gao, Xiang-Dong Li
Observations of elliptical galaxies suggest that black holes (BHs) might serve as dark energy candidates, coupled to the expansion of the Universe. According to this hypothesis, th…
Impact of Asymmetrical Mass Ejection from Proto-White Dwarfs on the Properties of Binary Millisecond Pulsars
Wen-Shi Tang, Shi-Jie Gao, Xiang-Dong Li
The standard formation theory of binary millisecond pulsars (BMSPs) predicts efficient orbital circularization due to tidal interaction during the previous mass transfer phase. The…
On the Magnetic Fields of Ultraluminous X-ray Pulsars
Shi-Jie Gao, Xiang-Dong Li
So far quite a few ultraluminous X-ray (ULX) pulsars have been discovered. In this work, we construct a super-Eddington, magnetic accretion disk model to estimate the dipole magnet…