Bo Wang
people.ucas.edu.cn
0000-0002-3231-1167
Yunnan Observatories, Chinese Academy of Sciences
58 papers found
Refreshing results…
Mass transfer of low-mass binaries and chemical anomalies among unevolved stars in globular clusters
Evolving neutron star+helium star systems to intermediate-mass binary pulsars
Circumstellar properties of Type Ia supernovae from the helium star donor channel
Off-centre carbon burning in He-accreting carbon–oxygen white dwarfs
Past and future of the central double-degenerate core of Henize 2–428
The progenitors of type-Ia supernovae in semidetached binaries with red giant donors
Optical and Radio Transients after the Collapse of Super-Chandrasekhar White Dwarf Merger Remnants
The outcomes of carbon–oxygen white dwarfs accreting CO-rich material
Stellar and AGN Feedback in Isolated Early-type Galaxies: The Role in Regulating Star Formation and ISM Properties
The single-degenerate model for the progenitors of accretion-induced collapse events
Mass-accreting white dwarfs and type Ia supernovae
Evolving ONe WD+He star systems to intermediate-mass binary pulsars
Accreting CO material onto ONe white dwarfs towards accretion-induced collapse
Carbon Stars Identified from LAMOST DR4 Using Machine Learning
The double-degenerate model for the progenitors of Type Ia supernovae
Merging of a CO WD and a He-rich WD to produce a type Ia supernovae
Discovery of Two New Hypervelocity Stars from the LAMOST Spectroscopic Surveys
He-accreting carbon–oxygen white dwarfs and Type Ia supernovae
Mass retention efficiencies of He accretion onto carbon-oxygen white dwarfs and type Ia supernovae
The core-degenerate scenario for the progenitors of Type Ia supernovae
Missing publications? Search for publications with a matching author name.