Pulsar-wind-induced disk heating in GRMHD simulations reproduces the high and low X-ray modes of transitional millisecond pulsars.
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Modes in Transitional Millisecond Pulsars: Evidence of Pulsar Wind-Induced Disk Heating from GRMHD and Radiative Transfer
Pulsar-wind-induced disk heating in GRMHD simulations reproduces the high and low X-ray modes of transitional millisecond pulsars.