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Modes in Transitional Millisecond Pulsars: Evidence of Pulsar Wind-induced Disk Heating from General-relativistic Magnetohydrodynamics and Radiative Transfer

  • Authors: Raphaël Mignon-Risse, Manuel Linares, Kyle Parfrey, Alexander Tchekhovskoy, Sean Ressler

Raphaël Mignon-Risse et al 2026 The Astrophysical Journal Letters 1010 .

  • Provider: AAS Journals

Caption: Figure C1.

Time evolution of the gas accretion torque (dashed line) and electromagnetic torque (full line) applied to the NS, normalized to the isolated value, in models sim-d36 (black) and sim-d100 (light blue).

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