期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 494, 期 1, 页码 L64-L68出版社
OXFORD UNIV PRESS
DOI: 10.1093/mnrasl/slaa038
关键词
stars: neutron; radio continuum: transients; (transients:) fast radio bursts; stars: black holes
资金
- AAS Foreign Travel Grant
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.
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