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Super-Chandrasekhar White Dwarfs by the Evolution of Magnetized Main-sequence Stars: New Mass Limits from STARS Simulation

  • Authors: Zenia Zuraiq, Banibrata Mukhopadhyay, Achal Kumar, Arnab Sarkar, Alexander J. Hackett, Projjwal Banerjee, Christopher A. Tout

Zenia Zuraiq et al 2026 The Astrophysical Journal Letters 1010 .

  • Provider: AAS Journals

Caption: Figure 2.

M–R curves showing different mass limits for different magnetic field profiles, i.e., different η (η and γ describe the magnetic field profile defined in Appendix A). ﹩\dot{M}=1{0}^{-9}\,{M}_{\odot }\,{{\rm{yr}}}^{-1}﹩ began at 1.02 M⊙ for all cases.

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