Astronomers first detected the new FRB, dubbed FRB 20240209A, in February 2024 with the Canadian Hydrogen Intensity Mapping Experiment (CHIME). Credit: CHIME, Andre Renard, Dunlap Institute for Astronomy & Astrophysics, University of Toronto.

A picture is emerging that shows maybe not all fast radio bursts come from young stars, with one traced to an old and dead elliptical galaxy.

For the first time, astronomers have traced a fast radio burst (FRB) to the outskirts of an ancient, dead, elliptical galaxy — an unprecedented home for a phenomenon previously associated with much younger galaxies.

Detailed in two complementary studies led by Northwestern University and McGill University, the discovery shatters assumptions that FRBs solely emanate from regions of active star formation.

The new observational evidence, instead, hints that the origins of these mysterious cosmic events might be more diverse than previously thought.

Northwestern’s Tarraneh Eftekhari, who led one of the studies and co-authored the other, said: “The prevailing theory is that FRBs come from magnetars formed through core-collapse supernovae.

“That doesn’t appear to be the case here. While young, massive stars end their lives as core-collapse supernovae, we don’t see any evidence of young stars in this galaxy.

“Thanks to this new discovery, a picture is emerging that shows not all FRBs come from young stars. Maybe there is a subpopulation of FRBs that are associated with older systems.”

Northwestern’s Wen-fai Fong, a senior author on both studies, added: “This new FRB shows us that just when you think you understand an astrophysical phenomenon, the Universe turns around and surprises us.

“This ‘dialogue’ with the Universe is what makes our field of time-domain astronomy so incredibly thrilling.”

A first for the CHIME outrigger telescopes

Astronomers first detected the new FRB, dubbed FRB 20240209A, in February 2024 with the Canadian Hydrogen Intensity Mapping Experiment (CHIME).

Flaring up and disappearing within milliseconds, FRBs are brief, powerful radio blasts that generate more energy in one quick burst than our Sun emits in an entire year.

But this event flared up more than once.

Between the initial burst in February through July 2024, the same source produced another 21 pulses — six of which were also detected by an outrigger telescope located 60km away from CHIME’s main station.

Smaller versions of CHIME, the outriggers enable astronomers to precisely confine the specific locations of FRBs on the sky.

The location of the fast radio burst, indicated by the oval outlines, is on the outskirts of a massive elliptical galaxy, the yellow oval at right. Credit: Gemini Observatory.

Most massive FRB host galaxy to date

After the team pinpointed the FRB’s position, Eftekhari and her collaborators hurried to use telescopes at the W.M. Keck and Gemini observatories to explore the event’s surrounding environment.

In a specialised room on the Evanston campus, Northwestern astronomers have remote access to Keck, which enables them to quickly observe phenomena of high interest. 

Instead of finding a young galaxy, these observations surprisingly revealed that the FRB originated at the edge of an 11.3-billion-year-old neighbouring galaxy, located just two billion lightyears from Earth.

To learn more about this unusual host galaxy, the team used high-performance computers to run simulations.

They found that the galaxy is extremely luminous and incredibly massive — 100 billion times the mass of our Sun.

Eftekhari said: “It seems to be the most massive FRB host galaxy to date. It’s among some of the most massive galaxies out there.”

A far-flung home

But, while most FRBs originate well within their galaxies, the team traced FRB 20240209A to the outskirts of its home — 130,000 lightyears from the galaxy’s centre where few other stars exist.

Vishwangi Shah, a graduate student at McGill, who led the effort to pinpoint the FRB’s origins, said: “Among the FRB population, this FRB is located the furthest from the centre of its host galaxy.

“This is both surprising and exciting, as FRBs are expected to originate inside galaxies, often in star-forming regions.

“The location of this FRB so far outside its host galaxy raises questions as to how such energetic events can occur in regions where no new stars are forming.”

‘Twinning’ FRBs

Before this discovery, astronomers had traced only one other FRB to the outer fringes of a galaxy.

In 2022, an international team of astronomers detected an FRB, which emanated from a tight cluster of stars on the edge of Messier 81 (M81), a grand design spiral galaxy located about 12 million light years from Earth.

Although FRB 20240209A occurred in an elliptical galaxy, the two events share several other similarities.

Fong said: “A few years ago, the M81 FRB was surprisingly discovered within a dense cluster of stars called a globular cluster.

“That event single-handedly halted the conventional train of thought and made us explore other progenitor scenarios for FRBs. Since then, no FRB had been seen like it, leading us to believe it was a one-off discovery — until now.” 

She added: “In fact, this CHIME FRB could be a twin of the M81 event. It is far from its home galaxy (far away from where any stars are being born), and the population of stars in its home galaxy is extremely old.

“It’s had its heyday and is now coasting into retirement. At the same time, this type of old environment is making us rethink our standard FRB progenitor models and turning to more exotic formation channels, which is exciting.”

Out of the nearly 100 FRBs that have been pinpointed to a galaxy so far, most have likely originated from magnetars, which are formed through core-collapse supernovae.

Astrophysicists posit FRB 20240209A’s origin, however, might be similar to the FRB found in M81.

Possible explanations

The McGill-led study discusses the likelihood that the new FRB originated within a dense globular cluster.

Such clusters are promising sites for magnetars possibly formed through other mechanisms and associated with older stars, including through the merger of two neutron stars or from a white dwarf collapsing under its own gravity.

Shah said: “A globular cluster origin for this repeating FRB is the most likely scenario to explain why this FRB is located outside its host galaxy.

“We do not know for a fact if there is a globular cluster present at the FRB position and have submitted a proposal to use the James Webb Space Telescope for follow-up observations of the FRB location.

“If yes, it would make this FRB only the second FRB known to reside in a globular cluster. If not, we would have to consider alternative exotic scenarios for the FRB’s origin.”

Eftekhari concluded: “It’s clear that there’s still a lot of exciting discovery space when it comes to FRBs, and that their environments could hold the key to unlocking their secrets.”

Both studies are published in the Astrophysical Journal Letters.