3 papers
astro-ph.SR2026
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…
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…