SIMBAD references

2016MNRAS.459.3307J - Mon. Not. R. Astron. Soc., 459, 3307-3313 (2016/July-1)

Ion-proton pulsars.

JONES P.B.

Abstract (from CDS):

Evidence derived with minimal assumptions from existing published observations is presented to show that an ion-proton plasma is the source of radio-frequency emission in millisecond and in normal isolated pulsars. There is no primary involvement of electron-positron pairs. This conclusion has also been reached by studies of the plasma composition based on well-established particle-physics processes in neutron stars with positive polar-cap corotational charge density. This work has been published in a series of papers which are also summarized here. It is now confirmed by simple analyses of the observed radio-frequency characteristics, and its implications for the further study of neutron stars are outlined.

Abstract Copyright: © 2016 The Author Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): plasmas - polarization - stars: neutron - pulsars: general - pulsars: general

Simbad objects: 18

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2021.06.15-03:20:16

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