Ph.D. candidate Cui Yingzhen and Prof. Meng Xiangcun from the Yunnan Observatories of the Chinese Academy of Sciences (CAS) performed hydrodynamic simulations on the common-envelope wind model of Type Ia supernovae (SNe Ia), and revealed the mass loss mechanism and the main observational features of white dwarf binaries in the common-envelope wind phase.
Click here for original story, Hydrodynamical simulations for the common-envelope wind model for Type Ia supernovae
Source: Phys.org