2022MNRAS.513.1925K


Query : 2022MNRAS.513.1925K

2022MNRAS.513.1925K - Mon. Not. R. Astron. Soc., 513, 1925-1931 (2022/June-3)

The absence of periodicity in repeating FRB.

KATZ J.I.

Abstract (from CDS):

Popular fast radio burst (FRB) models involve rotating magnetized neutron stars, yet no rotational periodicities have been found. Small data sets exclude exact periodicity in FRB 121102. Recent observations of over 1500 bursts from each of FRB 121102 and FRB 20201124A have also not found periodicity. Periodograms of events with cosine-distributed random offsets as large as ±0.6P from a strict period P would still reveal the underlying periodicity. The sensitivity of periodograms of long data series, such as bursts observed on multiple days, to slow frequency drifts is mitigated by considering individual observing sessions, and results are shown for FRB 121102. Models of repeating FRB without intrinsic periodicity are considered, as are models of apparently non-repeating FRBs.

Abstract Copyright: © 2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

Journal keyword(s): stars: black holes - stars: magnetars - accretion - accretion discs - radio continuum - transients: fast radio bursts

Simbad objects: 9

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Number of rows : 9
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 20190520B rB 16 02 04.270 -11 17 17.32           ~ 211 0
5 V* HZ Her LXB 16 57 49.8110126616 +35 20 32.486555472 11.90 14.89 13.63 13.88   B3/6ep 2172 0
6 PSR J1745-2900 Psr 17 45 40.1640 -29 00 29.818           ~ 358 0
7 PSR J1808-2024 Psr 18 08 39.32 -20 24 40.1           ~ 1316 2
8 SS 433 HXB 19 11 49.5647697480 +04 58 57.827127648   16.854 14.643     A7Ib 2253 4
9 FRB 200428 rB 19 35.0 +21 57           ~ 291 0

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