A team led by Sanchayeeta Borthakur of Arizona State University and Namrata Roy, now an assistant professor at the Raman Research Institute and a former ASU Exploration Prize Postdoctoral Fellow, has found evidence that narrow jets of heated plasma, blasted out by supermassive black holes, can reach far beyond the visible boundaries of their host galaxies and disrupt the gas those galaxies need to keep growing. The research, published in The Astrophysical Journal Letters, offers some of the clearest evidence yet that black holes can influence galactic environments on scales hundreds of thousands of light-years across, far beyond the compact region where the black hole itself resides.

The scale mismatch at the heart of this problem is staggering. A supermassive black hole, even an actively feeding one, occupies a region roughly the size of our solar system. Its host galaxy, by contrast, can contain around one hundred billion solar systems worth of stars and gas. When such a black hole feeds on infalling matter, it releases enormous amounts of energy that heat the surrounding gas, but how that energy travels outward and affects structures millions of times larger has remained one of the most persistent puzzles in astrophysics. Roy has compared the challenge to imagining an ant leaving its impression hundreds or thousands of kilometers away, a vivid illustration of just how disproportionate the influence appears to be.

The answer, according to the new work, lies in the jets themselves. Active black holes that emit strong jets launch narrow streams of hot, fast-moving plasma that shoot out far beyond a galaxy’s visible edge. Rather than spreading their energy equally in all directions, these jets act less like a lamp illuminating a room and more like a powerful beam that leaves a glowing trail wherever it passes. The team hypothesized that if jets truly penetrate the circumgalactic medium, they should leave a distinct imprint in the ionization state of the surrounding gas, a chemical and physical fingerprint written along the jet’s path.

Detecting that fingerprint was far from straightforward. The glow of ionized hydrogen in the CGM, observed through a specific emission feature known as H-alpha, is so faint that no single galaxy could reveal it clearly. To overcome this limitation, the researchers combined observations of hundreds of galaxies with active jets, drawing optical data from the Dark Energy Spectroscopic Instrument, or DESI, survey and radio jet measurements from the LOFAR Two-meter Sky Survey, known as LoTSS. By stacking the signals from many galaxies and aligning them along the directions of their radio jets, the team could search for a coherent H-alpha signal that would otherwise remain buried in noise.

The result was striking. When the stacked signal was averaged over all directions around the galaxies, it was weak and inconclusive. But when the astronomers looked specifically along the axes of the radio jets, the H-alpha signal became clear and strong. This directional pattern demonstrates that the gas does not glow uniformly around these galaxies; instead, it shines most brightly precisely where the jets pass through it. The jet ionizes hydrogen gas along its trajectory, lighting up a trail that extends deep into the circumgalactic medium and providing direct evidence that black hole energy reaches and transforms gas at enormous distances from the galactic center.

The study also mapped where the glow was strongest, and the answer revealed two distinct hotspots. The ionized hydrogen emission peaked close to the galaxy, where the jet first slams into the circumgalactic medium, and again much farther out near the CGM’s outer edge, where the jet deposits most of its remaining energy. This double-peaked structure offers a clear physical signature of how jets interact with their surroundings as they bore outward, illuminating and disrupting gas all the way from the inner boundary of the CGM to its farthest reaches.

As a crucial check on their interpretation, the team examined a completely different tracer: the absorption signature of magnesium, which traces cooler gas in the same regions. Unlike the strongly directional H-alpha glow, the magnesium signal was distributed isotropically, appearing equally in all directions with no connection to the jet orientation. This contrast suggests that the cool gas reservoir already surrounds the galaxy uniformly on all sides, while the jet selectively brightens, heats, and ionizes gas only along its own path. In other words, the jets are not creating the reservoir, but they are actively transforming it, carving an energized channel through an otherwise symmetric halo of fuel.

These findings carry profound implications for how galaxies live and die. By heating, stirring, and disturbing gas throughout the circumgalactic medium, jets can prevent that gas from cooling down and falling inward to fuel new stars. The mechanism acts as a brake on galactic growth, throttling star formation and potentially pushing a galaxy from an active, star-forming state into quiescence. The black hole, in this picture, is not merely a passive engine feeding at the center of its galaxy; it reaches outward and reshapes the galaxy’s entire environment, and in doing so it helps determine whether the galaxy continues to build stars or fades into quiet retirement. This feedback loop may finally explain why galaxies have not converted their abundant surrounding gas into far more stars than observations show.

The directional nature of the discovery is itself a methodological breakthrough. Previous searches for this signal failed to detect it, and the new study suggests why: the signal only appears when observations are aligned with the jet direction. Had the team assumed the circumgalactic medium was identical in every direction, the effect would have been averaged away and lost forever. The work also underscores the growing power of large optical and radio surveys such as DESI and LoTSS, which allow astronomers to combine many weak signals into detections of galactic behavior that would otherwise remain hidden. For theorists and observers alike, the result opens a new way to test how black hole jets affect galaxies, and, as Borthakur noted, a new direction for exploring the intricate connection between supermassive black holes trillions of miles away and the conditions that made life on Earth possible. Co-authors on the study include Timothy Heckman of Johns Hopkins University and Tanmay Singh of Arizona State University, with support from NASA, the Space Telescope Science Institute, and the National Science Foundation.

Subject of Research: The directional impact of supermassive black hole jets on the circumgalactic medium and galaxy evolution

Article Title: ASU astronomers uncover black hole jets reaching far beyond their galaxies and deciding their fate

Article References: ASU astronomers uncover black hole jets reaching far beyond their galaxies and deciding their fate. (n.d.). Original publication

Image Credits: AI Generated

DOI: Not provided

Keywords: supermassive black holes, black hole jets, circumgalactic medium, galaxy evolution, H-alpha emission, ionized gas, DESI survey, LOFAR, star formation, radio galaxies, astrophysics, galactic feedback