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astro-ph.HE2024
The threshold for pulsar radio emission is determined by the Goldreich-Julian charge density
P B Jones
A recent phenomenological study of radio emission from normal and millisecond pulsars by Karastergiou et al has lead these authors to state that they are unable to exclude a common…
astro-ph.HE2024
On the origin of the quasi-periodic micro-pulses observed in the radio-frequency emission of some neutron stars
P B Jones
The linear relationship between pulsar micro-pulse widths and rotation period is consistent with the existence of a physical length L on the neutron-star surface and seen on the ob…