2025ApJ...979L..41L


Query : 2025ApJ...979L..41L

2025ApJ...979L..41L - Astrophys. J., 979, L41 (2025/February-1)

Structure Functions of Rotation Measures Revealing the Origin of Fast Radio Bursts.

LI R.-N., ZHAO Z.-Y., WU Q., YI S.-X. and WANG F.-Y.

Abstract (from CDS):

Structure function (SF) analysis is a powerful tool for studying plasma turbulence. Theoretically, the SF of Faraday rotation measure (RM) is expected to include a geometric component due to the relative orientation of sight lines through an ordered magnetic field. However, observational evidence for this component remains elusive. Here, we report that the SFs of the binary PSR B1744-24A and the repeating fast radio burst (FRB) 20201124A exhibit both a periodic geometric component, caused by binary orbital motion, and a flat statistical component. The statistical component, induced by stochastic fluctuations in electron density and magnetic field, aligns with RM scatter derived from pulse depolarization. These findings indicate that FRB 20201124A has a binary origin and suggest that the periodic geometric component can serve as a diagnostic tool to identify binary companions.

Abstract Copyright: © 2025. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Radio transient sources - Magnetic fields - Interstellar medium - Radio bursts

Simbad objects: 8

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Number of rows : 8
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 20180916B rB 01 58 00.750 +65 43 00.30           ~ 457 0
2 FRB 20201124A rB 05 07 57.600 +26 11 24.00           ~ 307 0
3 FRB 20181119D rB 05 31 58.6980 +33 08 52.588           ~ 933 0
4 FRB 180301 rB 06 12 43.40 +04 33 44.8           ~ 125 0
5 FRB 20190303A G 13 51 59.77 +48 06 57.6           ~ 58 0
6 FRB 20190520B rB 16 02 04.270 -11 17 17.32           ~ 211 0
7 PSR B1744-24A Psr 17 48 02.249 -24 46 37.65           ~ 235 0
8 FRB 20220912A rB 23 09 04.9 +48 42 25           ~ 126 0

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