3 papers
astro-ph.SR2025
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…
astro-ph.SR2025
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…
astro-ph.SR2019
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…