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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 5.

Our simulations naturally exhibit an anticorrelation between the jet and X-ray emission. This can explain the observed radio–X-ray anticorrelation in the disk state. We distinguish data points corresponding to propeller (filled circles), wind (empty circles), and accretor (crosses) regimes. The anticorrelation is visible within each individual simulation.

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