Image Details

Choose export citation format:

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 B2.

Combinations of propeller and wind regimes in the sim-d100 model could reproduce the observed low-mode data. (a) Low-mode J1023 data (orange dots) and individual SEDs of the accretor, propeller, and wind (Rm > RLC) regimes. (b) Low-mode J1023 data (orange dots) and full SEDs (GRMHD data and star/disk models). (c) Low-mode J1023 data (orange dots) and combinations of the full SEDs between the accretor, propeller, and wind regimes. The data are best reproduced with the combination of 70% propeller and 30% wind regimes (sim-d100-p70-w30).

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse