How Supermassive Black Holes Feed Themselves

University of Michigan

An international research team using the JWST has found 'photographic evidence' that brings astronomers a step closer to solving a longstanding mystery about black holes

An image of elliptical galaxy NGC 4696 located at the center of the Centaurus Cluster taken by the Hubble Space Telescope. This image shows dusty, rust-colored filaments surrounding the bright yellow center of the galaxy.
An image of elliptical galaxy NGC 4696 located at the center of the Centaurus Cluster taken by the Hubble Space Telescope. This image shows dusty filaments surrounding the center of the galaxy. Image credit: NASA, ESA/Hubble, A. Fabian

Study: JWST Reveals How Black Holes are Fed: Kiloparsec-scale Multiphase Filaments Feed Subkiloparsec Circumnuclear Disks (DOI: 10.3847/2041-8213/ae81ae)

An international research team, including an astronomer from the University of Michigan, have revealed how certain black holes manage to eat and grow while simultaneously flinging their food across galaxies.

"We've found this almost smoking-gun, photographic evidence of how the black holes get their fuel, how they're getting this material to enlarge themselves," said Hyunseop "Joseph" Choi, postdoctoral researcher in the University of Michigan's Department of Astronomy.

Hyunseop
Hyunseop "Joseph" Choi

The research behind the discovery was led by the University of Montreal and enabled by the world's most powerful space telescope, the JWST. For this study, the JWST, a NASA mission developed in partnership with the Canadian Space Agency and the European Space Agency, observed a galaxy named NGC 4696 with a supermassive black hole at its center.

"We're finally seeing how gas falls back into a black hole for the first time with the state-of-the-art JWST observatory," said Choi, who began working on this project as a postdoctoral fellow at Montreal before joining Michigan.

Nearly every massive galaxy in the universe has a supermassive black hole at its core, millions or even billions of times more massive than the sun. When these black holes are actively pulling in surrounding material, they switch on like cosmic engines. They unleash powerful jets and winds of energy outward that can sculpt the entire galaxy around them, slowing down the birth of new stars and influencing how the galaxy grows over time. Astronomers call these types of black holes active galactic nuclei, or AGN.

A close-up of the center of galaxy NGC4696 around its supermassive black hole. The background greyscale imaging comes from the Hubble Space Telescope. The overlaid coloured map shows the distribution of gas falling into the black hole as traced by the Paschen α line using the JWST NIRSpec instrument. An S-shaped swirl can be seen in the gas. Image credit: NASA/ESA/CSA/STScI/J. Hlavacek-Larrondo et al. Astrophys. J. Lett. 2026. DOI: 10.3847/2041-8213/ae81ae
With JWST, researchers were also able to measure the velocity of the material near the supermassive black hole at the center of the galaxy NGC4696 (green circle). Measurements like these that are enabled by JWST play a key role in furthering our understanding of how black holes work. Although the black hole shoots hot material away from itself (arrow), cooler material falls back in, allowing the black hole to grow. Image credit: Image credit: NASA/ESA/CSA/STScI/J. Hlavacek-Larrondo et al. Astrophys. J. Lett. 2026. DOI: 10.3847/2041-8213/ae81ae
Astronomers using the JWST have recorded photographic evidence of material falling into the supermassive black hole at the core of an active galactic nucleus.

Despite extensive research, a puzzle has stumped scientists for years. If an AGN's jets heat up the surrounding gas, that should, in principle, shut off the black hole's food supply. So how does it keep feeding and growing?

The leading hypothesis is that the gas eventually cools back down, condenses into long thin streamers called filaments, and falls back toward the galaxy's center. The black hole thus feeds the process that then feeds the black hole. Despite decades of searching, directly observing how these filaments actually connect to the black hole has remained very difficult. That connection, a sort of missing link, is exactly what this new study reveals.

Julie Hlavacek-Larrondo
Julie Hlavacek-Larrondo

"What JWST is revealing is that black holes may be the ultimate cosmic recyclers," said Julie Hlavacek-Larrondo, a professor at the University of Montreal and lead author of the team's new study published in The Astrophysical Journal Letters.

"They release enormous amounts of energy that heat their surroundings, yet that same gas can later cool into thin filaments that fall back inward and feed the black hole again. We are finally seeing this self-sustaining cycle in action."

To test whether this explanation holds up, the team also ran computer simulations of the system. The simulated gas behaved in a way that closely matched what JWST observed, lending strong independent support to the proposed picture.

"It is exciting that JWST observations now allow us to directly test and constrain our simulations of black hole feeding, by comparing them to what we are seeing around a real black hole," said Minghao Guo, a doctoral student at Princeton University and co-author who led the simulations featured in the study.

A similar disk structure had previously been seen in another galaxy, NGC 1275 in the Perseus Cluster, using the ALMA Observatory. These new results in NGC 4696 suggest that this recycling mechanism may be common to massive galaxies across the universe.

"We've found just one example, so we're hoping to use JWST in the near future to see whether we can capture this kind of image from other black holes," Choi said. "I am very much looking forward to what our future JWST programs may reveal about how black holes feed themselves."

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