From AAS NOVA: “An Update on Fast Radio Bursts: New Discovery in Our Own Galaxy”



9 September 2020
Susanna Kohler

An artist’s rendering of an outburst on an ultra-magnetic neutron star. [NASA’s Goddard Space Flight Center.]

Have we recently spotted the first equivalent of a fast radio burst (FRB) — a mysterious and brief extragalactic flash of radio emission — in our own galaxy? Some astronomers think so, and argue that the new discovery solidifies the connection between these exotic radio bursts and powerfully magnetized neutron stars.

Origin of a Burst

Artist’s impression of telescopes observing an extragalactic fast radio burst. [CSIRO/Andrew Howells.]

Observations of bright, millisecond-duration, extragalactic radio flashes continue to pile up, yet the cause of these odd transients remains uncertain. One popular theory: FRBs may be somehow connected to the birth or evolution of magnetars, neutron stars threaded with especially strong magnetic fields.

There’s plenty of evidence pointing to magnetars as the source of FRBs, from polarization measurements that suggest FRB sources are strongly magnetized, to localizations of several FRBs to star-forming regions typical of magnetar environments. And some magnetars, known as soft gamma-ray repeaters (SGRs), emit repeated high-energy flares and bursts across their lifetime — another sign of volatility that could tie into the FRB picture.

But there’s a major challenge to the magnetar model for FRBs: we’ve never observed radio emission remotely similar to an FRB coming from a magnetar in our own galaxy.

…that is, until now.

A Missing Link Found?

In a new study led by Sandro Mereghetti (INAF, Italy), scientists have reported the detection of a series of bright X-ray bursts from the magnetar SGR 1935+2154 using the International Gamma-Ray Astrophysics Laboratory (INTEGRAL) spacecraft.


In itself, this announcement might not have been newsworthy — but the observed X-ray bursts from this known magnetar were also accompanied by a very bright millisecond radio burst detected by the Canadian Hydrogen Intensity Mapping Experiment (CHIME) and the Survey for Transient Astronomical Radio Emission 2 (STARE2) radio telescopes.

CHIME Canadian Hydrogen Intensity Mapping Experiment -A partnership between the University of British Columbia, the University of Toronto, McGill University, Yale and the National Research Council in British Columbia, at the Dominion Radio Astrophysical Observatory in Penticton, British Columbia, CA Altitude 545 m (1,788 ft).

The radio burst exhibits similar structure to the associated X-ray burst from the magnetar, occurred at roughly the same time, and is within a factor of 10 of the energy of some extragalactic FRBs. These clues strongly suggest that SGR 1935+2154’s outburst may be the missing link that connects magnetars with FRBs.

Pinpointing Production

Can we use these new observations of SGR 1935+2154 to narrow down models of FRB production?

In another recent study, Ben Margalit (NASA Einstein Fellow at UC Berkeley) and collaborators use the new data from this source first to argue that there must be two different populations of magnetars: “ordinary” magnetars like SGR 1935+2154 and other galactic magnetars, and more active but shorter lived magnetars that are responsible for cosmological FRBs. The latter population may form through different channels than galactic magnetars.

Margalit and collaborators also use the radio and X-ray observations from SGR 1935+2154 to evaluate specific magnetar emission mechanisms, providing constraints on models of how these energetic flashes are produced.

SGR 1935+2154 may have more X-ray and radio activity in store for us in the future, so you can bet we’ll be keeping an eye on it. With any luck, upcoming observations will help us to further address the mystery of FRBs — right here in our own galaxy.


“INTEGRAL Discovery of a Burst with Associated Radio Emission from the Magnetar SGR 1935+2154,” S. Mereghetti et al 2020 ApJL 898 L29.

“Implications of a Fast Radio Burst from a Galactic Magnetar,” Ben Margalit et al 2020 ApJL 899 L27.

See the full article here .


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