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2025MNRAS.537L..33J - Mon. Not. R. Astron. Soc., 537, L33-L35 (2025/February-2)
The threshold for pulsar radio emission is determined by the Goldreich-Julian charge density.
JONES P.B.
Abstract (from CDS):
Abstract Copyright: © 2024 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society.
Journal keyword(s): instabilities - plasmas - pulsars: general
CDS comments: PSR J1904+0056 is not identified.
Simbad objects: 33
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