2021MNRAS.506.4163L


Query : 2021MNRAS.506.4163L

2021MNRAS.506.4163L - Mon. Not. R. Astron. Soc., 506, 4163-4174 (2021/September-3)

GRB jet structure and the jet break.

LAMB G.P., KANN D.A., FERNANDEZ J.J., MANDEL I., LEVAN A.J. and TANVIR N.R.

Abstract (from CDS):

We investigate the shape of the jet break in within-beam gamma-ray burst (GRB) optical afterglows for various lateral jet structure profiles. We consider cases with and without lateral spreading and a range of inclinations within the jet core half-opening angle, θc. We fit model and observed afterglow light curves with a smoothly-broken power-law function with a free-parameter κ that describes the sharpness of the break. We find that the jet break is sharper (κ is greater) when lateral spreading is included than in the absence of lateral spreading. For profiles with a sharp-edged core, the sharpness parameter has a broad range of 0.1 <= κ <= 4.6, whereas profiles with a smooth-edged core have a narrower range of 0.1 <= κ <= 2.2 when models both with and without lateral spreading are included. For sharp-edged jets, the jet break sharpness depends strongly on the inclination of the system within θc, whereas for smooth-edged jets, κ is more strongly dependent on the size of θc. Using a sample of 20 GRBs, we find 9 candidate smooth-edged jet structures and 8 candidate sharp-edged jet structures, while the remaining 3 are consistent with either. The shape of the jet break, as measured by the sharpness parameter κ, can be used as an initial check for the presence of lateral structure in within-beam GRBs where the afterglow is well-sampled at and around the jet-break time.

Abstract Copyright: © 2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

Journal keyword(s): gamma-ray burst: general

Simbad objects: 28

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Number of rows : 28
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 GRB 080710 gB 00 33 05.68 +19 30 05.8           ~ 136 0
2 GRB 041006 gB 00 54 50.17 +01 14 07.0           ~ 202 2
3 SN 2009nz SN* 02 26 19.87 -18 57 08.6           ~ 307 1
4 GRB 061126 gB 05 46 24.460 +64 12 38.49 18.62 18.79 19.20     ~ 182 1
5 GRB 060729 gB 06 21 31.850 -62 22 12.69           ~ 303 0
6 SN 2003dh SN* 10 44 50.030 +21 31 18.15     16.2     SNIcpec 1261 1
7 SDSS J112848.22+170418.5 G 11 28 48.22989 +17 04 18.5014           ~ 393 0
8 SN 2013cq SN* 11 32 32.84 +27 41 56.2           SNIc 613 1
9 GRB 030226 gB 11 33 04.9 +25 53 56           ~ 212 0
10 GRB 050408 gB 12 02 17.320 +10 51 10.00           ~ 153 0
11 GRB 090426 G 12 36 18.0470 +32 59 09.460           ~ 237 0
12 GrW 170817 GWE 13 09 48.0850 -23 22 53.343           ~ 2683 0
13 GRB 060206 gB 13 31 43.420 +35 03 03.60   19.99 17.09     ~ 330 0
14 GRB 050801 gB 13 36 35.000 -21 55 41.00 15.03 15.82 15.46     ~ 164 0
15 GRB 990510 gB 13 38 07.64 -80 29 48.8           ~ 499 1
16 GRB 010222 G 14 52 12.5 +43 01 06           ~ 364 1
17 GRB 081203A gB 15 32 07.6 +63 31 15           ~ 177 0
18 GRB 060418 gB 15 45 42.600 -03 38 20.00 15.73 16.19 14.98     ~ 389 0
19 GRB 000301C gB 16 20 18.5 +29 26 35           ~ 361 0
20 GRB 080603A gB 18 37 37.95 +62 44 39.6           ~ 89 0
21 Fermi bn081008832 gB 18 39 52.40 -57 25 58.8           ~ 224 0
22 GRB 080413A gB 19 09 11.73 -27 40 39.6           ~ 163 0
23 GRB 090618 gB 19 36 01.80 +78 21 07.1           ~ 358 0
24 GRB 020813A gB 19 46 41.874 -19 36 04.81           ~ 316 0
25 GRB 050922C gB 21 09 33.000 -08 45 30.10 15.15 15.86 14.69     ~ 301 0
26 GRB 051109A gB 22 01 15.320 +40 49 23.70   20.09 20.14     ~ 190 0
27 GRB 050820A gB 22 29 38.110 +19 33 37.10 18.33 19.00 18.47     ~ 409 0
28 Fermi bn090926181 gB 23 33 36.18 -66 19 25.9           ~ 339 0

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