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Giant black holes from chaotic early era coming to light
Oct. 9, 2012
Courtesy of the Royal Astronomical Society
and World
Science staff
Cutting-edge sky surveys have revealed a previously unseen group of giant, fast-growing black holes from a violent early period in cosmic history, astronomers say.
Researchers claim the findings could have special significance because they shed light on how huge black holes and galaxies shaped each other’s early development.
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Astronomers say the red
dot is an image of the galaxy ULASJ1234+0907, 11 billion light years from Earth.
Dust obscures the object in the visible light, so this image was taken
using data from infrared light surveys (Credit: the UKIDSS and the Wide-field Infrared Survey Explorer
observatory)
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A black hole is an object so compact that its gravitational force becomes all-powerful in its region of space, and thus drags in anything that gets too close, including light.
Giant, or “supermassive,” black holes are believed to sit at the centers of galaxies, including our own.
The black holes described in the new research were previously undetected because thick layers of dust enshroud them. But they turn out to have been releasing copious radiation through violent interactions with their host galaxies, according to the authors of the new research.
Their report on the findings is to appear in the journal
Monthly Notices of the Royal Astronomical Society and is online
here.
The most extreme object in the study is a supermassive black hole called ULASJ1234+0907. This object, located in the direction of the constellation of Virgo, is so far away that the light from it has taken 11 billion years to reach us, so we see it as it appeared in the early universe. The monster black hole
is estimated to have more than 10 billion times the mass (weight) of the Sun and 10,000 times the mass of the supermassive black hole in our own Milky Way, making it one of the biggest black holes known.
But the research indicates there may be as many as 400 such giant black holes in the part of the universe that we can observe.
“These results could have a significant impact on studies of supermassive black holes,” said Manda Banerji of the University of Cambridge, lead author of the paper. “Most black holes of this kind are seen through the matter they drag in. As the neighbouring material spirals in towards the black holes, it heats up. Astronomers are able to see this radiation and observe these systems. Although these black holes have been studied for some time, the new results indicate that some of the most massive ones may have so far been hidden from our view.”
The newfound black holes, devouring the equivalent of several hundred Suns every year, are expected to shed light on the processes governing all supermassive black hole growth. By design, the sampled black holes come from a period “corresponding to the peak of star formation and black-hole” growth in our roughly 13.7-billion-year-old universe, the scientists wrote.
The most massive galaxies and their central black holes are widely believed to have grown through violent collisions with other galaxies, which trigger the formation of stars and provides food for the black holes to devour. These violent collisions would also have produced abundant dust, which briefly enshrouds the gorging black hole.
The most spectacular example already known of a dusty, growing black hole in the relatively nearby universe is the well-studied galaxy Markarian 231 located at a much smaller distance of 600 million light-years away, Banerji and colleagues said. A light-year is the distance light travels in a year. Studies with the Hubble Space Telescope indicate Markarian 231 crashed into another galaxy fairly recently in cosmic history.
ULASJ1234+0907 is being described as a more extreme version of this nearby galaxy, indicating conditions in the early
cosmos were much more turbulent and inhospitable than today.
The Cambridge researchers used infrared-light surveys being carried out on the U.K. Infrared Telescope to peer through the dust and locate the giant black holes for the first time. Infared light is a low-energy form of light not visible to the unaided eye. “These results are particularly exciting because they show that our new infrared surveys are finding super massive black holes that are invisible in optical surveys. These new quasars are important because we may be catching them as they are being fed through collisions with other galaxies,” said Richard McMahon at Cambridge, co-author of the study.
He added that observations with the new Atacama Large Millimeter Array telescope in Chile “will allow us to directly test this picture by detecting the microwave-frequency radiation emitted by the vast amounts of gas in the colliding galaxies.”
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Cutting-edge sky surveys using infrared light have revealed a previously unseen group of giant, fast-growing black holes from a violent early period in cosmic history, astronomers say.
Researchers claim the findings could have special significance because they shed light on how huge black holes and galaxies shaped each other’s early development.
A black hole is an object so compact that its gravitational force becomes all-powerful in its region of space, and thus drags in anything that gets too close, including light. Giant, or “supermassive,” black holes are believed to sit at the centres of galaxies, including our own.
The black holes described in the new research were previously undetected because thick layers of dust enshroud them. But they turn out to have been releasing copious radiation through violent interactions with their host galaxies, according to the authors of the new research. Their report is to appear in the journal Monthly Notices of the Royal Astronomical Society and is online here.
The most extreme object in the study is a supermassive black hole called ULASJ1234+0907. This object, located in the direction of the constellation of Virgo, is so far away that the light from it has taken 11 billion years to reach us, so we see it as it appeared in the early universe. The monster black hole has more than 10 billion times the mass of the Sun and 10,000 times the mass of the supermassive black hole in our own Milky Way, making it one of the biggest black holes known.
But the research indicates there may be as many as 400 such giant black holes in the part of the universe that we can observe.
“These results could have a significant impact on studies of supermassive black holes,” said Manda Banerji of the University of Cambridge, lead author of the paper. “Most black holes of this kind are seen through the matter they drag in. As the neighbouring material spirals in towards the black holes, it heats up. Astronomers are able to see this radiation and observe these systems. Although these black holes have been studied for some time, the new results indicate that some of the most massive ones may have so far been hidden from our view.”
The newfound black holes, devouring the equivalent of several hundred Suns every year, are expected to shed light on the processes governing all supermassive black hole growth. By design, the sampled black holes come from a period “corresponding to the peak of star formation and black-hole” growth in our roughly 13.7-billion-year-old universe, the scientists wrote.
The most massive galaxies and their central black holes are widely believed to have grown through violent collisions with other galaxies, which trigger the formation of stars and provides food for the black holes to devour. These violent collisions would also have produced abundant dust, which briefly enshrouds the gorging black hole.
The most spectacular, already known example of a dusty, growing black hole in the relatively nearby universe is the well-studied galaxy Markarian 231 located at a much smaller distance of 600 million light-years away, Banerji and colleagues said. A light-year is the distance light travels in a year. Studies with the Hubble Space Telescope indicate Markarian 231 crashed into another galaxy fairly recently in cosmic history.
ULASJ1234+0907 is being described as a more extreme version of this nearby galaxy, indicating conditions in the early Universe were much more turbulent and inhospitable than today.
The Cambridge researchers used infrared-light surveys being carried out on the U.K. Infrared Telescope to peer through the dust and locate the giant black holes for the first time. Infared light is a low-energy form of light not visible to the unaided eye. “These results are particularly exciting because they show that our new infrared surveys are finding super massive black holes that are invisible in optical surveys. These new quasars are important because we may be catching them as they are being fed through collisions with other galaxies,” said Richard McMahon at Cambridge, co-author of the study.
He added that observations with the new Atacama Large Millimeter Array telescope in Chile “will allow us to directly test this picture by detecting the microwave frequency radiation emitted by the vast amounts of gas in the colliding galaxies.”
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