Galaxy cluster extremely fertile: stars turned out fast thanks to a lazy central black hole.
"It should be producing less than one, and it's producing 740," says Michael McDonald of MIT, coauthor of a study describing the cluster in the Aug. 16 Nature.
Called "Phoenix" by the team for its location in the constellation Phoenix-its official name is SPT-CLJ2344-4243--the cluster comprises roughly 1,000 galaxies, is more than 4 million light-years across, and contains more mass than 2,000 Milky Ways.
In other words, it's big.
It's bright, too: The galactic conglomerate is the most luminous cluster ever observed in the X-ray spectrum. The star-birthing galaxy center is 50 times larger than the Milky Way. "It's kind of the boss galaxy," McDonald says.
The cluster's cold core and excessive fertility suggest the presence of a slacker black hole at the galaxy's center. Normally, radiation from a supermassive black hole--in this case, something around 10 billion times the mass of the sun--warms the surrounding environment, making it hard for gas to coalesce into stars. Whether this black hole is simply overworked, permanently off duty or just taking a break is unclear, but scientists think they've captured the cluster at an exceptionally frisky moment.
"Stars are forming at a much higher rate than we've seen before in any of these galaxies," says astrophysicist Martin Rees of the University of Cambridge in England. "It's a fascinating step toward putting this picture together of the tussle between the black holes and the star formation."
But the rate of star formation in the cluster may be somewhat overestimated, says astronomer Andrew Fabian, also at Cambridge. "There's no doubt that they've found a really exciting and fascinating object," he says. "Just how extreme it is, we don't know yet."
Astronomers discovered the riot of starbirth using the South Pole Telescope, a radio antenna that searches for the shadows cast by galaxy clusters on the cosmic microwave background, the thermal radiation left over from the Big Bang.
In the central galaxy, scientists are observing stars forming much faster than expected for a galaxy of this type. Calculating the stellar birthrate involves measuring the amount of X-rays emitted by gas as it cools off and falls toward the central galaxy. Though the swirling gas starts off at temperatures exceeding 10 million degrees Celsius, stars can't begin coalescing until it cools to temperatures nearer the ambient temperature of space--a few hundred degrees below zero.
Fabian and his colleagues suggested decades ago that star formation can proceed through such "cooling flows," but that process hadn't been observed in this type of central galaxy until now.
McDonald and his colleagues calculated that approximately 740 stars are bursting out of this central galaxy each year. But the sprinter's pace is unlikely to be a permanent feature of the cluster, because over a marathon distance it would produce a monster galaxy 1,000 times larger than anything ever observed.
It's more likely that scientists have captured the cluster in a fit of fertility, though it's unknown just how long that fit will last. "I think something around 100 million years is reasonable," McDonald says. Determining exactly how much gas--fuel for the fertile fire--is present will help resolve the timescale question. Scientists hope to make that measurement using the ALMA telescopes in northern Chile.
|Printer friendly Cite/link Email Feedback|
|Title Annotation:||Atom & Cosmos|
|Date:||Sep 22, 2012|
|Previous Article:||Back story: cave treasures.|
|Next Article:||Camera hack can find crime scene: simple infrared technology detects painted-over bloodstains.|