Imagine walking through the mall and seeing babies everywhere you looked. It would be a strange experience in part because, naturally, a sample of the population should include people at every stage of life. Now imagine that instead of looking at people in the mall, you are an astronomer observing galaxies in space. Perhaps these youngsters are not babies at all, but something different entirely.
A new investigation into an obscure class of galaxies known as Compact Symmetric Objects, or CSOs, has revealed that the objects are not entirely what they seem. CSOs are active galaxies that host supermassive black holes at their cores. Out of these monstrous black holes spring two jets traveling in opposite directions at nearly the speed of light. But in comparison to other galaxies that boast fierce jets, these jets do not extend out to great distances—they are much more compact. For many decades, astronomers suspected that CSOs were simply young and that their jets would eventually travel out to greater distances.
Now, reporting in three different papers in The Astrophysical Journal, a team of researchers led by Caltech has concluded that CSOs are not young but rather lead relatively short lives.
Greg Taylor, a Distinguished Professor of Physics and Astronomy at The University of New Mexico who worked on the research team, explained why the astronomers were not satisfied by the longstanding hypothesis that CSOs evolve into large radio galaxies over millions of years.
"One of the big problems with the CSOs is that there are just too many of them," Taylor says. "If you were looking at a slice of population then you'd expect to find old people, middle-aged people, young people, but you wouldn't expect to be outnumbered by the babies, right?"
The research group was determined to answer why they could not find CSOs older than around 5,000 years. It turns out the objects may not be baby versions of larger galaxies at all.
"These CSOs are not young," explains Anthony (Tony) Readhead, the Robinson Professor of Astronomy, Emeritus at Caltech, who led the investigation. "You wouldn't call a 12-year-old dog young even though it has lived a shorter life than an adult human. These objects are a distinct species all of their own that live and die out in thousands of years rather than the millions of years that are common in galaxies with bigger jets."
In the new studies, the team reviewed literature and past observations of more than 3,000 CSO candidates, verifying 64 as real and identifying an additional 15 CSOs. All these objects had been previously observed by the National Radio Astronomy Observatory's Very Long Baseline Array (VLBA), funded by the National Science Foundation (NSF), and some had been observed by other high-resolution radio telescopes. "The VLBA observations are the most detailed in astronomy, providing images with details equivalent to measuring the width of a human hair at a distance of 100 miles," Readhead says.
Evan Sheldahl, a UNM Ph.D. student of Physics with a concentration in Astrophysics, proposed the schedule for VLBA observations, calibrated data, and made images and spectral index maps for the research group. As the research into CSOs continues, he will help expand the sample of CSOs.
"With new high sensitivity observations of these sources, we hope to increase the current number of known CSOs by a substantial fraction and see if they support the theories we've developed about CSOs so far," Sheldahl says. "If what we've already learned from studying our meager sample of CSOs is any indication, I believe this research will have a great impact on our understanding of active galactic nuclei, supermassive black holes, and galaxy evolution."
The team's analysis concludes that CSOs expel jets for 5,000 years or less and then die out. "The CSO jets are very energetic jets but they seem to shut off," says Vikram Ravi, assistant professor of astronomy at Caltech and a co-author of one of the studies. "The jets stop flowing from the source."
As for what is fueling the short-lived jets, the scientists believe the cause is a tidal disruption event (TDE), which occurs when a single star wanders too close to a supermassive black hole and is devoured.
"We think that a single star gets ripped apart, and then all that energy is channeled into jets along the axis the black hole is spinning around," Readhead says. "The giant black hole starts out invisible to us, and then when it consumes a star, boom! The black hole has fuel, and we can see it."
Readhead first suspected that CSOs might be fueled by TDEs back in the 1990s, but he says the idea went largely unnoticed by the scientific community. "The hypothesis was all but forgotten because years went by before observational evidence began to mount for TDEs," he says. At the time of his original hypothesis, only three CSOs had been found.
Fast forward to 2020. Readhead, who had paused his studies of CSOs to delve into different problems in radio astronomy, decided it was time to revisit the topic. He gathered some of his colleagues together on Zoom, and they decided to comb through literature and weed out objects that had been misclassified as CSOs. Over the next two years, the team investigated more than 3,000 CSO candidates, narrowing the group down to only dozens that had the criteria to be real CSOs.
Ultimately, a picture began to emerge of CSOs as an entirely distinct family with jets that die out much sooner than their gigantic brethren, such as those of the extremely powerful Cygnus A, a galaxy that shoots out extremely powerful jets that glow brightly at radio wavelengths. These jets stretch to distances of about 230,000 light-years in each direction and last tens of millions of years. In contrast, the CSO jets extend to about 1,500 light-years at most and die out by about 5,000 years.
According to the astronomers, the CSO jets likely form when a supermassive black hole snacks on not just any star, but a substantial one.
"The TDEs we've previously seen only lasted for a few years," Ravi says. "We think that the remarkable TDEs powering CSOs last far longer because the disrupted stars are very large in size, very massive, or both."
By analyzing the varied collection of CSO radio images, the researchers say they can trace how the objects age over time, almost like looking at a photo album of a CSO's life to observe how its jets evolve. The younger CSOs have shorter jets that are closer to the black holes, while the older objects have jets that extend further out from their black hole. Though most of the jets die out, the scientists estimate that one in 100 will go onto to become long-lived like those of Cygnus A. In those rare cases, the galaxies are likely merging with other galaxies, a turbulent process that provides a large quantity of fuel.
If the discoveries of Readhead and his team are confirmed with additional observations, the CSOs will provide a whole new avenue for studying how massive stars at the centers of galaxies interact with supermassive black holes.
"These objects are indeed a distinct population with their own distinct origin, and it is up to us now to learn more about them and how they came to be," Readhead says. "Being able to study these objects on timescales of years to decades rather than millions of years has opened the door to a whole new laboratory for studying supermassive black holes and the many unexpected and unpredictable surprises they hold."
The three studies are, "Compact Symmetric Objects - I Towards a Comprehensive Bona Fide Catalog," "Compact Symmetric Objects – II Confirmation of a Distinct Population of High-Luminosity Jetted Active Galaxies," and "Compact Symmetric Objects – III Evolution of the High-Luminosity Branch and a Possible Connection with Tidal Disruption Events." The studies were funded by NSF, NASA, Caltech, and the Max Planck Institute for Radio Astronomy in Bonn, Germany.
Top image: This illustration shows how Compact Symmetric Objects, or CSOs, likely form. When a single, massive star wanders too close to a black hole (left), it is devoured and this causes the black hole to shoot out an ultrafast, bipolar jet (center). The jet extends outward and its hot ends glow with radio emissions (right). Image credit: NRAO/AUI/NSF
