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Chandra finds "piranha" black holes

Large amounts of active galactic nuclei, or supermassive black holes, thrive in young, distant galaxy clusters.
Provided by the Chandra X-ray Center, Cambridge, Massachusetts
This artist's conception shows a rapidly growing black hole, or an active galactic nucleus (AGN), at the center of a galaxy. A disk of hot gas is flowing into the central black hole and is surrounded by a large "doughnut" made up of cooler gas and dust.
NASA/CXC/M. Weiss
July 26, 2007
S upermassive black holes grow more rapidly in young galaxy clusters, according to new results from NASA's Chandra X-ray Observatory. These "fast-track," supermassive black holes can have a big influence on the galaxies and clusters they live in.

Using Chandra, scientists surveyed a sample of clusters and counted the fraction of galaxies with rapidly-growing, supermassive black holes, known as active galactic nuclei (AGN). The data show, for the first time, that younger, more distant galaxy clusters contained far more AGN than older, nearby ones.

Galaxy clusters are some of the largest structures in the universe, consisting of many individual galaxies, a few of which contain AGN. Earlier in the universe's history, these galaxies contained more gas for star formation and black hole growth than galaxies in clusters do today. This fuel allows the young-cluster black holes to grow much more rapidly than their counterparts in nearby clusters.

"The black holes in these early clusters are like piranha in a very well-fed aquarium," said Jason Eastman of Ohio State University and first author of the study. "It's not that they beat out each other for food; rather there was so much that all of the piranha were able to really thrive and grow quickly."

The team used Chandra to determine the fraction of AGN in four different galaxy clusters at large distances, when the Universe was about 58 percent of its current age. Then they compared this value to the fraction found in more nearby clusters, those about 82 percent of the universe's current age.

More-distant clusters contained about 20 times more AGN than the less-distant sample. AGN outside clusters are also more common when the universe is younger, but only by factors of two or three over the same age span.

"It's been predicted that there would be fast-track black holes in clusters, but we never had good evidence until now," said Paul Martini, co-author of the study. "This can help solve a couple of mysteries about galaxy clusters."

One mystery is why there are so many blue, star-forming galaxies in young, distant clusters and fewer in nearby, older clusters. AGN are believed to expel or destroy cool gas in their host galaxy through powerful eruptions from the black hole. This may stifle star formation and the blue, massive stars will then gradually die off, leaving behind only the old, redder stars. This process takes about a billion years or more to take place, so a dearth of star-forming galaxies is only noticeable for older clusters.

The process that sets the temperature of the hot gas in clusters when they form is also unknown. These new results suggest even more AGN may have been present when most clusters were forming about 10 billion years ago. Early heating of a cluster by large numbers of AGN can have a significant, long-lasting effect on the structure of a cluster by "puffing up" the gas.

"In a few nearby clusters we've seen evidence for huge eruptions generated by supermassive black holes. But this is sedate compared to what might be going on in younger clusters," said Eastman.
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