2016MNRAS.459.3307J

Query : 2016MNRAS.459.3307J

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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Number of rows : 18
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024 		#notes
1 PSR B0329+54 Psr 03 32 59.3370698592 +54 34 45.028206408           ~ 645 1
2 PSR B0355+54 Psr 03 58 53.7165 +54 13 13.727           ~ 437 1
3 PSR B0540+23 Psr 05 43 09.65 +23 29 06.1     14.40     ~ 253 0
4 PSR B0809+74 Psr 08 14 59.500 +74 29 05.70           ~ 406 0
5 PSR B0823+26 Psr 08 26 51.5068 +26 37 21.297           ~ 512 1
6 PSR B0834+06 Psr 08 37 05.642 +06 10 14.56           ~ 437 0
7 PSR B1133+16 Psr 11 36 03.0720 +15 51 15.500           ~ 668 0
8 PSR B1642-03 Psr 16 45 02.0330 -03 17 57.200           ~ 363 0
9 PSR B1706-16 Psr 17 09 26.4470 -16 40 56.200           ~ 222 0
10 AX J1809.8-1943 Psr 18 09 51.07 -19 43 51.8           ~ 463 0
11 PSR B1839+09 Psr 18 41 55.9380 +09 12 08.300           ~ 122 0
12 PSR B1916+14 Psr 19 18 23.638 +14 45 06.00           ~ 122 0
13 PSR B1919+21 Psr 19 21 44.815 +21 53 02.25           ~ 384 0
14 PSR B1929+10 Psr 19 32 14.0570 +10 59 33.380           ~ 753 0
15 PSR B1953+50 Psr 19 55 18.7637 +50 59 55.292           ~ 86 0
16 PSR B2020+28 Psr 20 22 37.0671 +28 54 23.104           ~ 306 1
17 PSR B2021+51 Psr 20 22 49.8730 +51 54 50.233           ~ 265 1
18 PSR B2111+46 Psr 21 13 24.3295 +46 44 08.844           ~ 208 1

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