SIMBAD references

2024MNRAS.532L..33J - Mon. Not. R. Astron. Soc., 532, L33-L35 (2024/July-3)

On the origin of the quasi-periodic micro-pulses observed in the radio-frequency emission of some neutron stars.

JONES P.B.

Abstract (from CDS):

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 observer arc of transit across the polar cap. Within the ion-proton model it is the width of the minimum area of surface that can support the critical growth rate of the unstable two-beam Langmuir mode that is the source of the radio emission.

Abstract Copyright: © 2024 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society.

Journal keyword(s): instabilities - plasmas - pulsars: general

Simbad objects: 29

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