2019ApJ...873..120Z

Query : 2019ApJ...873..120Z

2019ApJ...873..120Z - Astrophys. J., 873, 120-120 (2019/March-2)

A universal relation between the gamma-ray luminosity and power of relativistic outflows.

ZHU B.-T., ZHANG L. and FANG J.

Abstract (from CDS):

The relations between the gamma-ray luminosity and power for pulsar wind nebulae and short gamma-ray bursts are studied, respectively. After comparing with those for the previous relativistic outflow systems (including long gamma-ray bursts, active galactic nuclei, and black hole X-ray binaries), our results show that there exists a universal correlation between the gamma-ray luminosity and power, and the radiation efficiency is independent of the gamma-ray luminosity for various relativistic jet systems. Therefore, the acceleration and emission mechanisms or efficiencies may be similar in all relativistic outflows regardless of their central engines.

Abstract Copyright: © 2019. The American Astronomical Society. All rights reserved.

Journal keyword(s): gamma-ray burst: general - methods: statistical - pulsars: general - stars: winds, outflows

Simbad objects: 29

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Number of rows : 29
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 SNR G119.5+10.2 SNR 00 06.6 +72 47           ~ 268 1
2 PSR J0007+7303 Psr 00 07 00.6000137 +73 03 06.849976           ~ 183 1
3 SNR G130.7+03.1 SNR 02 05 35.73 +64 49 41.3           ~ 661 4
4 PSR J0205+6449 Psr 02 05 37.92 +64 49 42.8           ~ 268 1
5 M 1 SNR 05 34 31.8 +22 01 03           ~ 6516 1
6 V* CM Tau Psr 05 34 31.9474694616 +22 00 52.153698024           ~ 5476 0
7 PSR J0537-6910 Psr 05 37 46.66 -69 10 17.1           ~ 309 1
8 NGC 2060 SNR 05 37 51.4466169456 -69 10 23.947092084   9.69 9.59     ~ 380 2
9 PSR B0540-69 Psr 05 40 11.2000490438 -69 19 54.198559829           ~ 976 3
10 NAME Vela SNR 08 34.0 -45 50           ~ 1331 2
11 PSR J1119-6127 Psr 11 19 14.30 -61 27 49.5           ~ 439 1
12 PSR J1124-5916 Psr 11 24 37.6 -59 16 20           ~ 178 1
13 SNR G292.0+01.8 SNR 11 24 59 -59 19.1           ~ 351 1
14 PSR J1301-6305 Psr 13 02 47.9992676 -63 10 48.001099           ~ 139 2
15 GrW 170817 GWE 13 09 48.0850 -23 22 53.343           ~ 2683 0
16 PSR J1357-6429 Psr 13 57 02.525 -64 29 29.89           ~ 171 1
17 SNR G310.6-01.6 SNR 14 00 45.69 -63 25 42.6           ~ 45 1
18 PSR J1418-6058 Psr 14 18 42.725 -60 58 01.89           ~ 129 0
19 PSR J1420-6048 Psr 14 20 08.190 -60 48 14.85           ~ 214 0
20 PSR J1509-5850 Psr 15 09 27.153 -58 50 56.05           ~ 131 0
21 3A 1510-590 Psr 15 13 17.000 -59 04 54.00           ~ 434 3
22 PSR B1509-58 Psr 15 13 47.6 -59 07 54     13.06     ~ 879 1
23 SNR G000.9+00.1 SNR 17 47.3 -28 09           ~ 222 1
24 NAME AGPS 273.4-17.8 SNR 18 13 35.05 -17 49 58.1           ~ 145 2
25 SNR G021.5-00.9 SNR 18 33 33.612 -10 34 07.69           ~ 490 1
26 SNR G029.7-00.3 SNR 18 46 22.8 -02 59 47           ~ 375 2
27 PSR J1846-0258 Psr 18 46 24.75 -02 58 29.6           ~ 388 2
28 SNR G054.1+00.3 SNR 19 30 10.6 +18 50 22           ~ 271 1
29 PSR J1930+1852 Psr 19 30 30.13 +18 52 14.1           ~ 110 1

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