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A Supermassive Black Hole Gets Blamed for Quenching Star Formation
Some of the most massive galaxies in the Universe appear to be missing a lot of stars. That seems unusual, since birthing stars is one of a galaxy’s main tasks as it grows. According to Xin “Cindy” Xiang of the University of Michigan, something is suppressing or quenching the births of stars in these galaxies, and she thinks that black holes might be the culprit.
Xiang led a team of researchers who used the X-Ray Imaging and Spectroscopy Mission (XRISM) to study outflows from the accretion disks of black holes. Such regions are bright in X-rays, due to the fantastically high energies expended by material in the disks. Depending on the strength of winds coming from the region, they may play a very important role in affecting star formation. However, the team needed extremely high-resolution spectral studies of the emissions from the black hole to understand what was happening. “Previously, without XRISM, we could only see broad features of the outflows,” Xiang said. “But you need to be able to resolve fine features to answer important questions. What is their structure and geometry? How are the winds launched and when are they launched?”
Creating an Environment that Suppresses Stars
Supermassive black holes, like their smaller counterparts (the stellar-mass black holes), feed on material that gets caught in their strong gravitational pull. That includes light, as well as gas, dust, and anything bigger (such as stars) that tends to stray too close. The material swirls in through an accretion disk that forms around the black hole. The disk, particularly around a supermassive one, is an incredibly energetic environment. The activity there mixes gas and dust particles, and the whole thing is threaded through with magnetic fields. All that motion creates friction, and gravity works as well to atomize the material.
If things are energetic enough, they can even peel electrons off of those atoms, creating a very hot, very bright plasma. Like a bubbling cauldron, this disk can also fling out material, creating powerful winds. If the winds are strong enough, they can blow away gas in nearby regions. Unfortunately, that gas is what galaxies need to form new stars. So, black holes can have a pretty deleterious effect on the starbirth activity nearby.
Catching the Black Hole’s Outflow
Xiang and her team used XRISM to study activity near the supermassive black hole at the heart of galaxy NGC 4151. It supplied a high-resolution look at the winds flowing from the accretion disk at the heart of this active galactic nucleus (AGN) and measured their characteristics. AGN typically occur during a supermassive black hole’s growth phase, and their energetic activities shape the evolution of the host galaxy. They grow by gobbling up gas, as well as influencing surrounding gas clouds. They emit those powerful energetic winds during the growth phase.
This is what’s happening in the core of NGC 4151 as it gorges on nearby material and creates the accretion disk. “With XRISM, we have the greatest resolution observing the brightest AGN, and we’re getting the richest information on outflows that we have observed so far for an accretion disk,” Xiang said.
A Hubble Space Telescope view of the galaxy NGC 4151. Note the bright blue regions of starbirth out in the spiral arms, while there are relatively few regions near the core. Credit: NASA, ESA, Joseph DePasquale (STScI)
What XRISM Tells Us
It turns out that the strongest winds that shape the galaxy and eat up the gas that stars need to form don’t flow all the time. Xiang had to come up with a way to understand when those winds are the strongest. So, she analyzed hundreds of days of NGC 4151 observations, looking for peaks in X-ray brightness that would indicate strong winds.
An illustration of the winds and accretion disk around a supermassive black hole that makes up an AGN. Credit: NASA/M.Weiss (Chandra X-ray Center)
In addition, she looked at how hard or soft the X-rays were detected by XRISM so she could correlate them with wind strength. She put all these variables into a metric that she called the “color intensity index”, or “cindicity”. “Partly because my name is Cindy,” Xiang said. “But the idea is that, in the future, you could tell me the cindicity of your source at this moment and I can tell you the probability that you’re seeing a fast outflow.”
For NGC 4151, Xiang found the fast winds were strongest when the X-rays were hard but faint. The fastest winds were not seen during flares, but typically about 10,000 seconds—or just under 3 hours later—providing the first direct timing link to the outflows.
How Winds Affect Star Formation
As mentioned, the principal effect of an AGN on surrounding gas clouds in a galaxy is pretty catastrophic for starbirth regions. The winds can simply blow the gas away, dispersing it throughout the galaxy or into intergalactic space. If it’s spread out widely enough, there won’t be enough in any given region to begin the process of star formation. The winds can also shred the gas molecules, which also affects star formation.
The black hole’s main activity, gobbling down material, also removes the available star formation material completely. The result is the same: no gases to coalesce into stars. In turn, the galaxy loses its chance to grow through star formation.
Xiang’s team found multiple types of disk winds in the outflows from NGC 4151. All of these outflows had outflow rates that were equal to or greater than the mass accretion rate, meaning they were blowing essential material away. The team’s measurements and conclusions about the winds flowing from this galaxy’s supermassive black hole will help astronomers predict when such outflows are happening in other galaxies. That, in turn, could enhance scientists’ understanding of AGNs across the Universe.
For More Information
Revealing How and When a Black Hole’s Mighty Winds Can Squash Star Formation
XRISM Spectroscopy of Accretion-driven Wind Feedback in NGC 4151
News
Two Million X-Ray Sources, and One Cluster That Doesn’t Fit
Clusters are the largest gravitationally bound things in the universe, thousands of galaxies held together in a vast reservoir of hot gas, gas so hot it glows in X-rays rather than visible light. But they do not stop at a tidy, neat edge. They taper away into the surrounding darkness, and they are still being fed, drawing in fresh material along enormous threads of gas that run between them like the strands of a web. Those outskirts are the interesting part, because they are where the universe is still assembling itself. They are also very faint, which is why so little is known about them.
The eROSITA telescope, launched in 2019 aboard the joint Russian and German Spektrum-RG mission, has now published its second major data release. Built from three complete surveys of the sky, DR2 contains close to two million X-ray sources across the western half of the sky, about twice as many as the first release. Roughly 1.9 million are point like, mostly stars and feeding supermassive black holes. Some 64,000 are extended: galaxy clusters, nearby galaxies and the shredded remains of supernovae.

Galaxy cluster A3266 in X-rays, linked by a filament of hot gas to a neighbouring galaxy group. The Bonn team measured the faint outer glow for the first time and found gas hotter and denser than the models predict (Credit : Jakob Dietl/Uni Bonn/eROSITA-DE)
Within that haul, Thomas Reiprich and Jakob Dietl at Bonn’s Argelander Institute went after a single object. A3266 is a massive cluster connected by a filament of gas to a neighbouring group of galaxies, and their team became the first to measure the faint X-ray glow in its outer reaches.
Our current theories of how cosmic structure formed match what eROSITA sees, that’s reassuring. The interesting news is in the detail, where they don’t quite match. The gas in the outskirts and in the filament runs hotter and denser than predicted, and contains comparatively little in the way of heavy elements.

The Perseus cluster, one of the brightest X-ray objects in the sky. The diffuse glow is gas hot enough to shine in X-rays, and it holds more mass than all the cluster’s stars together (Credit : X-ray: NASA/CXC/SAO/V. Olivares et al.; Optical/IR: DSS; H-alpha: CFHT/SITELLE; Image Processing: NASA/CXC/SAO/N. Wolk)
Heavy elements, anything past hydrogen and helium, are manufactured inside stars and flung out when those stars die. Gas that is short of them has therefore never spent much time near a galaxy, which marks it as relatively pristine material arriving from the wider cosmic web rather than something expelled from the cluster itself. Yet it’s warmer and denser than models predict for gas of that kind. The two facts pull against each other, and reconciling them means adjusting our picture of how matter actually falls into a cluster: how quickly it heats, how thoroughly it mixes with what is already there and how much enriched gas the galaxies push back out to meet it.
Before eROSITA, the only X-ray survey of the whole sky came from ROSAT in 1990, so astronomers waited the best part of three decades for a successor. And eROSITA itself has been in safe mode since February 2022, with no return to science operations. There is a lesson in that about the value of surveying everything, whether or not you know yet what you are looking for.
Source : Homing In on the X-Ray Sky
News
L.A. reaches deal on cost recovery for 2028 Olympics, amid warnings

A divided Los Angeles City Council finalized a deal with organizers of the 2028 Summer Olympic Games aimed at controlling the city’s costs during the global event, amid complaints that the protections don’t go far enough.
On a 10-4 vote, the council approved the Enhanced City Resources Master Agreement, which lays out the process for the city to seek reimbursement for the services it provides during the Games.
City Administrative Officer Matt Szabo said the agreement sets up additional financial safeguards, by allowing the city to tap a $270-million contingency fund set up by LA28, the privately run Olympic organizing committee, if outstanding costs remain.
Still, some on the council warned that taxpayers could wind up on the hook for $1 billion in police and other public safety costs if LA28 incurs serious losses.
“This fails to provide any safeguards for Los Angeles taxpayers and most assuredly risks the city’s fiscal stability,” Councilmember Monica Rodriguez said after voting against the agreement. Councilmembers Eunisses Hernandez, Ysabel Jurado and Nithya Raman, who is running against Mayor Karen Bass, also were opposed.
Critics of the Games have long voiced concern about the risks that surround the event.
If LA28 incurs massive financial losses, the city would cover the first $270 million. The state would absorb the next $270 million. After that, the city’s general fund, which pays for basic services, would cover any remaining shortfall.
The city’s negotiating team said L.A.’s political leaders committed the city roughly a decade ago to serve as a financial backstop for the Games, as part of the contract that made L.A. the host city.
“We are providing you today as many protections as we can, given the reality that if it is not financially successful, it does fall onto us,” Szabo said. “So there is nothing we could propose today or tomorrow or next year that would eliminate that risk.”
The council, in a flurry of votes, sidelined proposals from Councilmembers Imelda Padilla, Hernandez and Raman that were billed as a way to reduce the risk facing the city.
LA28 spokesperson Jacie Prieto Lopez, in a statement, said the newly approved agreement delivers on the committee’s commitment to “execute a safe, secure and fiscally responsible Games that benefit Los Angeles for decades to come.”
Under the terms approved by the council, LA28 would pay the city ahead of the Games for services that are ineligible for reimbursement from the federal government, such as street sweeping and deployment of traffic officers.
The terms around police protection are more complicated.
The city would first seek reimbursement from the federal government for law enforcement services, particularly in high-security zones, Szabo said. If the government fails to cover the cost of security in those areas, the city would seek all or a portion of LA28’s contingency funds to make up difference, he said.
Last year, President Trump signed the One Big Beautiful Bill Act, setting aside $1 billion for state and local governments for security, planning and other costs associated with the Games.
Some council members have voiced concerns that the federal government might not follow through on its commitment, or that only a fraction of those funds would make their way to L.A., one of several Southern California communities slated to host Olympic competitions.
In April, Rodriguez sent LA28 a letter warning the city’s public safety costs could easily blow past $1 billion if there is an emergency or major weather event.
City Controller Kenneth Mejia, in an interview, said he intends to use his office to look into LA28’s finances in the run-up to the Games. He also argued that the deal to secure the Olympics was a bad one from the beginning.
“We’re already locked into a huge financial liability. This was one of our big chances to throw in protections for the city and also provide that transparency,” said Mejia, who opposed the agreement.
If LA28 makes money on the Games, the organizing committee would be barred from distributing that surplus to any organization until it has covered its financial obligations to the city, according to the terms approved Wednesday by the council.
Szabo, appearing before the council, acknowledged that the city faces a financial risk. If LA28 does experience a financial loss, it first would tap its own $330-million contingency fund, he said.
After that, LA28 and the city would have access to a second, $270-million contingency fund set up to protect taxpayers, he said.
“Is that a likely scenario? We don’t believe so,” Szabo said. “Their reports thus far have suggested that they are meeting their targets on their sponsorships and on other revenues, and we want them to continue to hit their targets.”
Those arguments haven’t satisfied an array of activists, who urged the council to rewrite the agreement.
“LA28 has no incentive to keep the city from being forced into bankruptcy,” said Chris Tyler, spokesperson for Strategic Actions for a Just Economy, a nonprofit that advocates for low-income communities in L.A.
Under a deal reached in 2021, LA28 must reimburse the city for services that go beyond what would be provided on a normal day in key parts of the city, such as Exposition Park, the Sepulveda Basin and parts of downtown L.A.
The organizing committee is obligated to create a $270-million contingency fund that can be distributed as a surplus if the Games make money or cover any losses in the event of a shortfall.
The proposal approved Wednesday calls for the five-year-old agreement to be amended to ensure that those contingency funds can be used to cover the city’s costs in the event that other funds aren’t available.
The city and LA28 were supposed to have a draft agreement on the cost recovery process completed by October. A draft document did not surface until June.
City negotiators now head into another round of talks with LA28 on the precise level of services needed at the Convention Center, Venice Beach, Dodger Stadium and other locations. Those venue agreements must be completed in July 2027.
Under the terms approved Wednesday, the two sides must reach an accord on the cost of those additional services by October 2027.
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