4 citations · 9 across the 4 of their papers we have counts for
4 papers
Mass-Orbital Period Distribution of Massive White Dwarfs Formed Through Stable Mass Transfer
Rizhong Zheng, Hongwei Ge, Christopher A Tout +10
White dwarfs (WDs) in binaries can form through either the stable mass-transfer process or common envelope evolution (CEE). Compared to CEE, the stable mass-transfer process can le…
Producing type Ia supernovae from hybrid CONe white dwarfs with main-sequence binary companions at low metallicity of Z = 0.0001
Boyang Guo, Xiangcun Meng, Zhijia Tian +2
The nature of progenitors of Type Ia supernovae (SNe Ia) and their explosion mechanism remain unclear. It has been suggested that SNe Ia may be resulted from thermonuclear explosio…
Using Lithium and Beryllium to Study Structure and Evolution of Rotating Stars
Wuming Yang, Haibo Yuan, Yaqian Wu +2
The chemical composition of the Sun is still a highly controversial issue. No solar model has yet been able to simultaneously reproduce the solar lithium and beryllium abundances,…
Solar Models and Astrophysical S-factors Constrained by Helioseismic Results and Updated Neutrino Fluxes
Wuming Yang, Zhijia Tian
The ratio of metal abundance to hydrogen abundance of the solar photosphere, , has been revised several times. Standard solar models, based on these revised solar abunda…