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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 C1.

Profiles showing change of temperature from center to surface for a few different magnetized WDs of different mass. Here, magnetic field profile is given by η = 1.1, γ = 0.9. 

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