2020MNRAS.497.1382Q


Query : 2020MNRAS.497.1382Q

2020MNRAS.497.1382Q - Mon. Not. R. Astron. Soc., 497, 1382-1390 (2020/September-2)

A population analysis of pulse broadening in ASKAP fast radio bursts.

QIU H., SHANNON R.M., FARAH W., MACQUART J.-P., DELLER A.T., BANNISTER K.W., JAMES C.W., FLYNN C., DAY C.K., BHANDARI S. and MURPHY T.

Abstract (from CDS):

The pulse morphology of fast radio bursts (FRBs) provides key information in both understanding progenitor physics and the plasma medium through which the burst propagates. We present a study of the profiles of 33 bright FRBs detected by the Australian Square Kilometre Array Pathfinder. We identify seven FRBs with measureable intrinsic pulse widths, including two FRBs that have been seen to repeat. In our modest sample, we see no evidence for bimodality in the pulse width distribution. We also identify five FRBs with evidence of millisecond time-scale pulse broadening caused by scattering in inhomogeneous plasma. We find no evidence for a relationship between pulse broadening and extragalactic dispersion measure. The scattering could be either caused by extreme turbulence in the host galaxy or chance propagation through foreground galaxies. With future high time resolution observations and detailed study of host galaxy properties, we may be able to probe line-of-sight turbulence on gigaparsec scales.

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

Journal keyword(s): methods: data analysis - intergalactic medium - galaxies: ISM - fast radio bursts

Simbad objects: 33

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Number of rows : 33
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 FRB 170707 rB 02 59.0 -57 16           ~ 16 0
2 FRB 171216 rB 03 28.0 -57 04           ~ 14 0
3 FRB 180119 rB 03 29.3 -12 44           ~ 16 0
4 FRB 171116 rB 03 31.0 -17 14           ~ 16 0
5 FRB 171213 rB 03 39.0 -10 56           ~ 18 0
6 FRB 180324 rB 06 16.0 -34 47           ~ 15 0
7 FRB 180430 rB 06 51.0 -09 57           ~ 10 0
8 FRB 170107 rB 11 23 10 -05 01.0           ~ 27 0
9 FRB 171004 rB 11 57.6 -11 54           ~ 15 0
10 FRB 190714 rB 12 15 55.1 -13 01 16           ~ 64 0
11 FRB 180417 rB 12 24 56 +14 13.0           ~ 6 0
12 FRB 171003 rB 12 29.5 -14 07           ~ 15 0
13 FRB 20180128A rB 13 56.0 -06 43           ~ 15 0
14 FRB 180212 rB 14 21.0 -03 35           ~ 16 0
15 FRB 180525 rB 14 40.0 -02 12           ~ 14 0
16 FRB 180315 rB 19 35.0 -26 50           ~ 12 0
17 FRB 190611 rB 21 22 58.91 -79 23 51.3           ~ 82 0
18 FRB 190102 rB 21 29 39.76 -79 28 32.5           ~ 83 0
19 FRB 180924 rB 21 44 25.255 -40 54 00.10           ~ 140 0
20 FRB 170428 rB 21 47.0 -41 51           ~ 16 0
21 FRB 181112 rB 21 49 23.630 -52 58 15.39           ~ 131 0
22 FRB 180131 rB 21 49.9 -40 41           ~ 14 0
23 FRB 180130 rB 21 52.2 -38 34           ~ 15 0
24 FRB 180110 rB 21 53.0 -35 27           ~ 21 0
25 FRB 20190711A rB 21 57 40.7 -80 21 29           ~ 114 0
26 FRB 170906 rB 21 59.8 -19 57           ~ 16 0
27 FRB 170416 rB 22 13.0 -55 02           ~ 16 0
28 FRB 171020 rB 22 15.0 -19 40           ~ 54 0
29 FRB 190608 rB 22 16 04.74 -07 53 53.6           ~ 102 0
30 FRB 171019 rB 22 17.5 -08 40           ~ 52 0
31 HIDDEN NAME FRB 180128.2 rB 22 22.0 -60 15           ~ 15 0
32 FRB 170712 rB 22 36.0 -60 57           ~ 15 0
33 FRB 180515 rB 23 13 12.0 -42 14 46           ~ 8 0

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