Could a radio flare in a nearby galaxy be a sign of a star being torn apart by a supermassive black hole?
Credit:ESO/M. Kornmesser
Credit:ESO/M. Kornmesser
Astronomers have seen an extraordinarily bright, long-lasting radio flare in the center of a nearby galaxy. After investigating further they found evidence of a relativistic jet most likely caused by the immense gravitational pull of the galaxy’s supermassive black hole tearing a star apart.
Credit: NRAO/AUI/NSF
An Unusual Signal
A team led by Jean Somalwar (California Institute of Technology) made the initial discovery by trawling through two archived radio surveys of the sky conducted decades apart. Between 1993 and 2018, a radio flare designated VT J0243 appeared in the nucleus of a nearby galaxy, growing one hundred times brighter over this time and continuing to brighten even now.
Intrigued, Somalwar and colleagues conducted a series of follow-up observations across multiple parts of the electromagnetic spectrum. Radio observations revealed the presence of a powerful relativistic jet. The spectrum of the jet revealed it to be young. Whatever caused it must have happened fairly recently.
X-ray analysis hinted at the presence of an accretion disk of material in the galactic center. Matter falling from this disk into the black hole could account for the radio flares, and material corralled by the black hole’s magnetic field could launch the jet.
Active galactic nuclei can light up the radio sky — but VT J0243 doesn’t quite fit with a typical active galaxy picture.
Credit: NASA/JPL-Caltech
Credit: NASA/JPL-Caltech
Exploring the Options
The team examined two main possibilities for what happened. The first suggests a long-standing accretion disk that existed long before the flare was fired — in other words, this galaxy is an active galactic nucleus. However, if this picture is correct, the team says it isn’t clear what caused the accretion rate to suddenly spike and generate the flare. The energy distribution across the radio spectrum also differs from most other active galactic nuclei with young jets. If it is an active galactic nucleus, it would be an unusual one.
The second option is that a star passed too close to the black hole and was ripped apart in what’s known as a tidal disruption event. However, there was no X-ray flare associated with this event — and astronomers have only seen one jetted tidal disruption event without such a flare before. It would also have taken an unusually long time for the radio emission to start after the tidal disruption event.
For now it remains a mystery, but this discovery is a clarion call for astronomers ahead of an influx of data from the Very Large Array Sky Survey (VLASS). Started in 2017 and due to finish in 2024, this survey is trawling 80% of the sky and is expected to catalog approximately 10 million radio sources. Among them should be many young jets like the one associated with VT J0243. Perhaps then astronomers will better understand the true triggers of such dramatic radio flares.
The second option is that a star passed too close to the black hole and was ripped apart in what’s known as a tidal disruption event. However, there was no X-ray flare associated with this event — and astronomers have only seen one jetted tidal disruption event without such a flare before. It would also have taken an unusually long time for the radio emission to start after the tidal disruption event.
For now it remains a mystery, but this discovery is a clarion call for astronomers ahead of an influx of data from the Very Large Array Sky Survey (VLASS). Started in 2017 and due to finish in 2024, this survey is trawling 80% of the sky and is expected to catalog approximately 10 million radio sources. Among them should be many young jets like the one associated with VT J0243. Perhaps then astronomers will better understand the true triggers of such dramatic radio flares.
Artist’s impression of a tidal disruption event — the ripping apart of a star by a black hole.
Credit: NASA/JPL-Caltech
Credit: NASA/JPL-Caltech
Citation
“A Candidate Relativistic Tidal Disruption Event at 340 Mpc,” Jean J. Somalwar et al 2023 ApJ 945 142. doi:10.3847/1538-4357/acbafc
