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Cited article:

The C/O ratio of He-accreting carbon-oxygen white dwarfs and type Ia supernovae

Xiao Cui, Bo Wang, Cheng-Yuan Wu, Xiang-Cun Meng and Zhan-Wen Han
Research in Astronomy and Astrophysics 20 (1) 003 (2020)
https://doi.org/10.1088/1674-4527/20/1/3

Hydrogen and helium shell burning during white dwarf accretion

Xiao Cui, Xiang-Cun Meng and Zhan-Wen Han
Research in Astronomy and Astrophysics 18 (5) 058 (2018)
https://doi.org/10.1088/1674-4527/18/5/58

CXO J004318.8+412016, a steady supersoft X-ray source in M 31

Marina Orio, G. J. M. Luna, R. Kotulla, et al.
Monthly Notices of the Royal Astronomical Society 470 (2) 2212 (2017)
https://doi.org/10.1093/mnras/stx1355

Quark-novae in neutron star - white dwarf binaries: a model for luminous (spin-down powered) sub-Chandrasekhar-mass Type Ia supernovae?

Rachid Ouyed and Jan Staff
Research in Astronomy and Astrophysics 13 (4) 435 (2013)
https://doi.org/10.1088/1674-4527/13/4/006

The influence of chemical composition on models of Type Ia supernovae

Alan C. Calder, Brendan K. Krueger, Aaron P. Jackson and Dean M. Townsley
Frontiers of Physics 8 (2) 168 (2013)
https://doi.org/10.1007/s11467-013-0301-4

Type-Ia Supernova Rates and the Progenitor Problem: A Review

D. Maoz and F. Mannucci
Publications of the Astronomical Society of Australia 29 (04) 447 (2012)
https://doi.org/10.1071/AS11052