2021MNRAS.500.1708R

Query : 2021MNRAS.500.1708R

2021MNRAS.500.1708R - Mon. Not. R. Astron. Soc., 500, 1708-1720 (2021/January-2)

Searching for the radio remnants of short-duration gamma-ray bursts.

RICCI R., TROJA E., BRUNI G., MATSUMOTO T., PIRO L., O'CONNOR B., PIRAN T., NAVAIEELAVASANI N., CORSI A., GIACOMAZZO B. and WIERINGA M.H.

Abstract (from CDS):

Neutron star mergers produce a substantial amount of fast-moving ejecta, expanding outwardly for years after the merger. The interaction of these ejecta with the surrounding medium may produce a weak isotropic radio remnant, detectable in relatively nearby events. We use late-time radio observations of short duration gamma-ray bursts (sGRBs) to constrain this model. Two samples of events were studied: four sGRBs that are possibly in the local (<200 Mpc) Universe were selected to constrain the remnant non-thermal emission from the sub-relativistic ejecta, whereas 17 sGRBs at cosmological distances were used to constrain the presence of a proto-magnetar central engine, possibly re-energizing the merger ejecta. We consider the case of GRB 170817A/GW170817 and find that in this case the early radio emission may be quenched by the jet blast-wave. In all cases, for ejecta mass range of Mej≲10–2 (5×10–2) M☉, we can rule out very energetic merger ejecta Eej≳5×1052 (1053) erg, thus excluding the presence of a powerful magnetar as a merger remnant.

Abstract Copyright: © 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): gamma-ray burst: general - stars: magnetars - stars: neutron

Simbad objects: 46

goto Full paper

goto View the references in ADS

Number of rows : 46
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 QSO B0019+058 BLL 00 22 32.44121084 +06 08 04.2689202   19.2   19.07   ~ 152 1
2 ICRF J002914.2+345632 Sy2 00 29 14.24247204 +34 56 32.2470345   20.2       ~ 145 1
3 GRB 070810B gB 00 35 48.4 +08 49 18           ~ 57 0
4 LEDA 1354367 G 00 35 53.4391562832 +08 49 27.354862596           ~ 9 0
5 Fermi bn150120123 G 00 41 16.5630 +33 59 42.598           ~ 70 0
6 QSO J0125-0006 Bla 01 25 28.8438355224 -00 05 55.930595964   16.92 16.64 16.30   ~ 305 1
7 GRB 130822A gB 01 51 41.27 -03 12 31.7           ~ 34 0
8 PSO J047.1631+13.1580 G 03 08 39.14930640 +13 09 29.0253240           ~ 144 0
9 QSO B0306+101 Bla 03 09 03.62349423 +10 29 16.3409179   18.45   19.91   ~ 214 1
10 IC 328 EmG 03 31 10.941 -14 38 16.47   14   13.90   ~ 32 0
11 GRB 050906 gB 03 31 15.28 -14 36 30.1           ~ 76 1
12 QSO B0338-214 BLL 03 40 35.60785848 -21 19 31.1721373   16.04 17.1 17.07   ~ 182 1
13 GRB 061006 G 07 24 07.8080 -79 11 55.188           ~ 214 0
14 GRB 080121 gB 09 08 56.0 +41 50 29           ~ 40 0
15 SDSS J090858.15+414926.5 G 09 08 58.16 +41 49 26.5           ~ 3 0
16 SDSS J090904.12+415033.2 G 09 09 04.1285093592 +41 50 33.149233176           ~ 4 0
17 6C 091740+445437 Bla 09 20 58.45848666 +44 41 53.9850947   18.40 18.16 16.55   ~ 407 1
18 GRB 150424A gB 10 09 13.35 -26 37 51.2           ~ 94 0
19 LEDA 86918 G 10 17 00.259 +35 31 18.91   17.5       ~ 11 0
20 Fermi bn100216422 gB 10 17 03 +35 31.0           ~ 32 0
21 7C 1015+3557 Bla 10 18 10.98810472 +35 42 39.4409041   18.62 18.07 17.65   ~ 212 1
22 QSO B1034-293 Bla 10 37 16.07974265 -29 34 02.8134977   16.46 16.46 17.54   ~ 358 1
23 ICRF J112027.8+142054 Sy2 11 20 27.80814059 +14 20 54.9730732   20 20.935 20.100   ~ 175 1
24 SDSS J112848.22+170418.5 G 11 28 48.22989 +17 04 18.5014           ~ 393 0
25 7C 1219+2830 BLL 12 21 31.6904439888 +28 13 58.500308172   16.81 16.11 14.24   ~ 924 1
26 GALEX J123205.0-105600 Bz? 12 32 04.9717245480 -10 56 00.722548932         16.421 ~ 186 0
27 SDSS J123612.87+285858.8 BiC 12 36 12.8803407000 +28 58 58.780075656           ~ 328 1
28 QSO J1246-0730 Bla 12 46 04.23211565 -07 30 46.5746985   17.6 18.0 18.2   ~ 198 1
29 QSO B1256-220 Bla 12 58 54.47878185 -22 19 31.1250428   19.16 20 19.20   ~ 121 1
30 GrW 170817 GWE 13 09 48.0850 -23 22 53.343           ~ 2683 0
31 GRB 140903A G 15 52 03.2650 +27 36 10.710           ~ 138 0
32 ICRF J160913.3+264129 Sy2 16 09 13.3196 +26 41 29.042   19       ~ 249 1
33 4C 51.37 Bla 17 40 36.97784792 +52 11 43.4073694   18.16 18.70 16.73   ~ 441 1
34 GRB 060502B gB 18 35 46.060 +52 37 51.45           ~ 153 1
35 Fermi bn160821937 gB 18 39 54.550 +62 23 30.35           ~ 190 0
36 Fermi bn080905499 G 19 10 42.0450 -18 52 54.510           ~ 200 0
37 QSO B1908-202 Bla 19 11 09.65289294 -20 06 55.1090664   18.21   18.14   ~ 306 1
38 6C 192647+611105 BLL 19 27 30.4428785736 +61 17 32.878880988   17.5 17.5 16.99   ~ 139 1
39 GRB 060614 G 21 23 32.140 -53 01 36.10           ~ 714 0
40 GRB 060505 gB 22 07 03.440 -27 48 51.89           ~ 286 1
41 GRB 061201 gB 22 08 32.060 -74 34 47.90           ~ 205 0
42 Fermi bn090510016 G 22 14 12.6230 -26 34 58.550           ~ 548 0
43 PKS 2211-388 rG 22 14 38.56966 -38 35 45.0098           ~ 34 1
44 GRB 080123 gB 22 35 46.100 -64 54 03.24           ~ 98 0
45 NVSS J230126-385839 rG 23 01 26.7650 -38 58 40.422   22.22 21.22 21   ~ 325 1
46 NAME Local Group GrG ~ ~           ~ 9325 0

To bookmark this query, right click on this link: simbad:objects in 2021MNRAS.500.1708R and select 'bookmark this link' or equivalent in the popup menu