2 citations · 2 across the 5 of their papers we have counts for
5 papers
A compact object with a K type star companion in the solar neighborhood: a wide post common envelope binary with a white dwarf candidate
Jie Lin, Hailiang Chen, Bojun Wang +3
Post-common envelope binaries (PCEBs) consisting of a white dwarf (WD) plus a main-sequence (MS) star can constrain current prescriptions of common envelope evolution (CEE) and cal…
The orbital period changes for novae
Wenshi Tang, Xiangdong Li, Bo Wang
Cataclysmic variable (CVs) are close interacting binaries in which a white dwarf accretes materials from a low mass main sequence companion. CVs can experience nova eruptions due t…
Eclipsing millisecond pulsars with He star companions
Yunlang Guo, Bo Wang, Xiangdong Li +2
Eclipsing millisecond pulsars (MSPs) are a type of pulsar binaries with close orbits (d). They are important objects for studying the accretion history of neutron st…
Formation of millisecond pulsars with wide orbits
Bo Wang, Dongdong Liu, Yunlang Guo +4
Millisecond pulsars (MSPs) are a kind of radio pulsars with short spin periods, playing a key role in many aspects of stellar astrophysics. In recent years, some more MSPs with wid…
Evolving neutron star+helium star systems to intermediate-mass binary pulsars
Tang Wenshi, Liu Dongdong, Wang Bo
Intermediate-mass binary pulsars (IMBPs) are composed of neutron stars (NSs) and CO/ONe white dwarfs (WDs). It is generally suggested that IMBPs evolve from intermediate-mass X-ray…