2014MNRAS.445..770J

Query : 2014MNRAS.445..770J

2014MNRAS.445..770J - Mon. Not. R. Astron. Soc., 445, 770-777 (2014/November-3)

The mechanism of coherent radio emission in some classes of pulsar.

JONES P.B.

Abstract (from CDS):

Radio luminosities have been estimated from published data for a well-defined homogeneous set of 29 normal pulsars. The radio frequency energies per unit charge in the primary accelerated particle beam are given for each pulsar and form a distribution more than two orders of magnitude in width. The values found show that pulsars are extremely efficient generators of radiation below 1-10 GHz given the kinematic constraints which are obtained here in the cases of electron-positron and ion-proton plasmas. Our conclusion is that only the ion-proton plasma source is consistent with the spectra of normal and millisecond pulsars and we list and describe the factors which together support this conclusion.

Abstract Copyright: © 2014 The Author Published by Oxford University Press on behalf of the Royal Astronomical Society (2014)

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

Simbad objects: 32

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Number of rows : 32
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 PSR B0031-07 Psr 00 34 08.9100 -07 21 56.000           ~ 350 0
2 PSR B0138+59 Psr 01 41 39.938 +60 09 32.30     12.85     ~ 120 0
3 PSR B0320+39 Psr 03 23 26.6619 +39 44 52.403           ~ 139 0
4 PSR B0329+54 Psr 03 32 59.3370698592 +54 34 45.028206408           ~ 690 1
5 PSR J0437-47 Psr 04 37 15.7994581776 -47 15 08.544351636           DC 1032 0
6 PSR B0525+21 Psr 05 28 52.308 +22 00 01.00     14.30     ~ 370 0
7 V* CM Tau Psr 05 34 31.9474694616 +22 00 52.153698024           ~ 5476 0
8 PSR B0628-28 Psr 06 30 49.35000 -28 34 42.1000           ~ 313 1
9 PSR B0809+74 Psr 08 14 59.500 +74 29 05.70           ~ 425 0
10 PSR B0818-13 Psr 08 20 26.40700 -13 50 56.3200           ~ 229 0
11 PSR B0823+26 Psr 08 26 51.5068 +26 37 21.297           ~ 541 1
12 PSR B0834+06 Psr 08 37 05.64620 +06 10 15.8700           ~ 472 0
13 PSR B0919+06 Psr 09 22 13.85000 +06 38 19.0000           ~ 329 1
14 PSR B1133+16 Psr 11 36 03.09460 +15 51 15.9000           ~ 715 0
15 PSR B1237+25 Psr 12 39 40.386 +24 53 49.87           ~ 497 1
16 PSR B1508+55 Psr 15 09 25.674 +55 31 32.90           ~ 322 1
17 PSR B1604-00 Psr 16 07 12.078 -00 32 40.98           ~ 228 1
18 PSR B1642-03 Psr 16 45 02.0330 -03 17 57.200           ~ 394 0
19 AX J1809.8-1943 Psr 18 09 51.07 -19 43 51.8           ~ 532 0
20 PSR B1845-01 Psr 18 48 23.59600 -01 23 58.4800           ~ 154 0
21 PSR B1911-04 Psr 19 13 54.16240 -04 40 47.5600           ~ 192 0
22 PSR B1929+10 Psr 19 32 14.0570 +10 59 33.380           ~ 801 0
23 PSR B1933+16 Psr 19 35 47.7011639352 +16 16 40.034899524           ~ 328 1
24 PSR B1944+17 Psr 19 46 53.044 +18 05 41.24           ~ 252 0
25 PSR B2016+28 Psr 20 18 03.8999255016 +28 39 54.940329468           ~ 374 0
26 PSR B2021+51 Psr 20 22 49.8730 +51 54 50.233           ~ 288 1
27 PSR B2044+15 Psr 20 46 39.33600 +15 40 33.6000           ~ 109 0
28 PSR B2045-16 Psr 20 48 35.74000 -16 16 45.0000           ~ 344 0
29 PSR B2111+46 Psr 21 13 24.3295 +46 44 08.844           ~ 226 1
30 PSR B2154+40 Psr 21 57 01.840 +40 17 45.89           ~ 155 0
31 PSR B2319+60 Psr 23 21 55.213 +60 24 30.71     13.80     ~ 200 0
32 PSR B2351+61 Psr 23 54 04.7830 +61 55 46.845           ~ 102 0

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