2022MNRAS.510.1801S


Query : 2022MNRAS.510.1801S

2022MNRAS.510.1801S - Mon. Not. R. Astron. Soc., 510, 1801-1808 (2022/February-3)

Statistical similarity between soft gamma repeaters and repeating fast radio bursts.

SANG Y. and LIN H.-N.

Abstract (from CDS):

We study the statistical properties of the soft gamma repeater SGR 1935+2154. We find that the cumulative distributions of duration, waiting time, fluence, and flux can be well fitted by bent power law. In addition, the probability density functions of fluctuations of duration, waiting time, fluence, and flux well follow the Tsallis q-Gaussian distribution. The q values keep steady for different temporal scale intervals, indicating a scale-invariant structure of the bursts. Those features are very similar to the property of the repeating fast radio burst FRB 121102, indicating the underlying association between the origins of soft gamma repeaters and repeating fast radio bursts.

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

Journal keyword(s): stars: individual: SGR J1935+2154 - stars: magnetars - fast radio bursts

Simbad objects: 5

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Number of rows : 5
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 20181119D rB 05 31 58.6980 +33 08 52.588           ~ 933 0
2 PSR J1550-5418 Psr 15 50 54.18 -54 18 23.9           ~ 463 1
3 PSR J1808-2024 Psr 18 08 39.32 -20 24 40.1           ~ 1316 2
4 NAME Sgr 1935+2154 * 19 34 55.68 +21 53 48.2           ~ 820 1
5 FRB 200428 rB 19 35.0 +21 57           ~ 291 0

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