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Chandra suggests black holes gorging at excessive rates

This finding may help astronomers understand how the largest black holes were able to grow so rapidly in the early universe.
RELATED TOPICS: BLACK HOLES | QUASARS
The black holes in these quasars may be growing at an extraordinarily rapid rate.
A new Chandra study indicates the existence of a population of black holes that is consuming extremely large amounts of material. Thick, donut-shaped disks may be surrounding the black holes, blocking much of the light that would otherwise be emitted. The black holes in these quasars may be growing at an extraordinarily rapid rate.
X-ray: NASA/CXC/Penn State/B.Luo et al.; Illustration: NASA/CXC/M.Weiss
A group of unusual giant black holes may be consuming excessive amounts of matter, according to a new study using NASA’s Chandra X-ray Observatory. This finding may help astronomers understand how the largest black holes were able to grow so rapidly in the early universe.

Astronomers have known for some time that supermassive black holes — with masses ranging from millions to billions of times that of the Sun and residing at the centers of galaxies — can gobble up huge quantities of gas and dust that have fallen into their gravitational pull. As the matter falls toward these black holes, it glows with such brilliance that they can be seen billions of light-years away. Astronomers call these extremely ravenous black holes “quasars.”

This new result suggests that some quasars are even more adept at devouring material than scientists previously knew.

“Even for famously prodigious consumers of material, these huge black holes appear to be dining at enormous rates, at least five to 10 times faster than typical quasars,” said Bin Luo of Penn State University in State College.

Luo and his colleagues examined data from Chandra for 51 quasars that are located at a distance between about 5 billion and 11.5 billion light-years from Earth. These quasars were selected because they had unusually weak emission from certain atoms, especially carbon, at ultraviolet wavelengths. About 65 percent of the quasars in this new study were found to be much fainter in X-rays, by about 40 times on average, than typical quasars.

The weak ultraviolet atomic emission and X-ray fluxes from these objects could be an important clue to the question of how a supermassive black hole pulls in matter. Computer simulations show that at low inflow rates matter swirls toward the black hole in a thin disk. However, if the rate of inflow is high, the disk can puff up dramatically because of pressure from the high radiation into a torus, or doughnut, that surrounds the inner part of the disk.

“This picture fits with our data,” said Jianfeng Wu of the Harvard-Smithsonian Center for Astrophysics in Cambridge, Massachusetts. “If a quasar is embedded in a thick doughnut-shaped structure of gas and dust, the doughnut will absorb much of the radiation produced closer to the black hole and prevent it from striking gas located further out, resulting in weaker ultraviolet atomic emission and X-ray emission.”

The usual balance between the inward pull of gravity and the outward pressure of radiation would also be affected.

“More radiation would be emitted in a direction perpendicular to the thick disk, rather than along the disk, allowing material to fall in at higher rates,” said Niel Brandt of Penn State University.

The important implication is that these “thick-disk” quasars may harbor black holes growing at an extraordinarily rapid rate. The current study and previous ones by different teams suggest that such quasars might have been more common in the early universe, only about a billion years after the Big Bang. Such rapid growth might also explain the existence of huge black holes at even earlier times.
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