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Strange signal near Milky Way’s centre has scientists stumped

- WORDS BRANDON SPECKTOR

Astronomer­s have detected a strange, repeating radio signal near the centre of the Milky Way, and it’s unlike any other energy signature ever studied. The energy source is extremely finicky, appearing bright in the radio spectrum for weeks at a time and then completely vanishing within a day. This behaviour doesn’t quite fit the profile of any known type of celestial body, the researcher­s wrote in their study, and thus may represent “a new class of objects being discovered through radio imaging”.

The radio source, known as ASKAP J173608.2-321635, was detected with the Australian Square Kilometre Array Pathfinder (ASKAP) radio telescope, situated in the remote Australian outback. In an ASKAP survey taken between April 2019 and August 2020, the strange signal appeared 13 times, never lasting in the sky for more than a few weeks. This radio source is highly variable, appearing and disappeari­ng with no predictabl­e schedule, and it doesn’t seem to appear in any other radio telescope data prior to the ASKAP survey.

When the researcher­s tried to match the energy source with observatio­ns from other telescopes, including the Chandra X-ray Observator­y and the Neil Gehrels Swift Observator­y, as well as the Visible and Infrared Survey Telescope for Astronomy in Chile, which can pick up near-infrared wavelength­s, the signal disappeare­d entirely.

With no apparent emissions in any other part of the electromag­netic spectrum, ASKAP J173608.2-321635 is a radio ghost that seems to defy explanatio­n. Prior surveys have detected low-mass stars that periodical­ly flare-up with radio energy, but those flaring stars typically have X-ray counterpar­ts. That makes a stellar source unlikely here.

Dead stellar remnants, like pulsars and magnetars – two types of ultradense, collapsed stars – are also unlikely explanatio­ns. While pulsars can stream bright beams of radio light past Earth, they spin with predictabl­e periodicit­y, usually sweeping their lights past our telescopes on a timescale of hours, not weeks. Magnetars, meanwhile, always include a powerful X-ray counterpar­t with each of their outbursts – again unlike ASKAP J173608.2-321635’s behaviour.

The closest match is a mysterious class of object known as a galactic centre radio transient (GCRT), a rapidly glowing radio source that brightens and decays near the Milky Way’s centre, usually over the course of a few hours. So far only three GCRTS have been confirmed, and all of them appear and disappear much more quickly than this new ASKAP object does.

However, the few known GCRTS do shine with a similar brightness as the mysterious signal, and their radio flare-ups are never accompanie­d by X-rays. If this new radio object is a GCRT, its properties push the boundaries of what astronomer­s thought GCRTS were capable of. Future radio surveys of the galactic centre should help clear up the mystery.

 ?? ?? The centre of the Milky Way, captured by the Spitzer Space Telescope’s infrared cameras
The centre of the Milky Way, captured by the Spitzer Space Telescope’s infrared cameras

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