A fast radio burst associated with a Galactic magnetar

C. D. Bochenek (), V. Ravi, K. V. Belov, G. Hallinan, J. Kocz, S. R. Kulkarni and D. L. McKenna
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C. D. Bochenek: California Institute of Technology
V. Ravi: California Institute of Technology
K. V. Belov: California Institute of Technology
G. Hallinan: California Institute of Technology
J. Kocz: California Institute of Technology
S. R. Kulkarni: California Institute of Technology
D. L. McKenna: California Institute of Technology

Nature, 2020, vol. 587, issue 7832, 59-62

Abstract: Abstract Since their discovery in 20071, much effort has been devoted to uncovering the sources of the extragalactic, millisecond-duration fast radio bursts (FRBs)2. A class of neutron stars known as magnetars is a leading candidate source of FRBs3,4. Magnetars have surface magnetic fields in excess of 1014 gauss, the decay of which powers a range of high-energy phenomena5. Here we report observations of a millisecond-duration radio burst from the Galactic magnetar SGR 1935+2154, with a fluence of 1.5 ± 0.3 megajansky milliseconds. This event, FRB 200428 (ST 200428A), was detected on 28 April 2020 by the STARE2 radio array6 in the 1,281–1,468 megahertz band. The isotropic-equivalent energy released in FRB 200428 is 4 × 103 times greater than that of any radio pulse from the Crab pulsar—previously the source of the brightest Galactic radio bursts observed on similar timescales7. FRB 200428 is just 30 times less energetic than the weakest extragalactic FRB observed so far8, and is drawn from the same population as the observed FRB sample. The coincidence of FRB 200428 with an X-ray burst9–11 favours emission models that describe synchrotron masers or electromagnetic pulses powered by magnetar bursts and giant flares3,4,12,13. The discovery of FRB 200428 implies that active magnetars such as SGR 1935+2154 can produce FRBs at extragalactic distances.

Date: 2020
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DOI: 10.1038/s41586-020-2872-x

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