2020MNRAS.494L..64K

Query : 2020MNRAS.494L..64K

2020MNRAS.494L..64K - Mon. Not. R. Astron. Soc., 494, L64-L68 (2020/May-1)

Are fast radio bursts made by neutron stars?

KATZ J.I.

Abstract (from CDS):

Popular models of repeating fast radio bursts (FRBs; and perhaps of all FRBs) involve neutron stars because of their high rotational or magnetostatic energy densities. These models take one of two forms: giant but rare pulsar-like pulses like those of rotating radio transients, and outbursts like those of soft gamma repeaters. Here I collate the evidence, recently strengthened, against these models, including the absence of Galactic micro-FRBs, and attribute the 16 d periodicity of FRB 180916.J0158+65 to the precession of a jet produced by a massive black hole's accretion disc.

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

Journal keyword(s): stars: neutron - radio continuum: transients - (transients:) fast radio bursts - stars: black holes

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 20181119D rB 05 31 58.6980 +33 08 52.588           ~ 933 0
3 FRB 190523 rB 13 48 15.6 +72 28 11           ~ 109 0
4 V* HZ Her LXB 16 57 49.8110126616 +35 20 32.486555472 11.90 14.89 13.63 13.88   B3/6ep 2172 0
5 PSR J1808-2024 Psr 18 08 39.32 -20 24 40.1           ~ 1316 2
6 SS 433 HXB 19 11 49.5647697480 +04 58 57.827127648   16.854 14.643     A7Ib 2253 4
7 HD 226868 HXB 19 58 21.6757355952 +35 12 05.784512688 9.38 9.72 8.91 8.42   O9.7Iabpvar 4590 0
8 FRB 180924 rB 21 44 25.255 -40 54 00.10           ~ 140 0

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