Giant Black Holes Devouring Huge Amounts Of Matter

A group of unusual giant black holes seems to be eating up excessive amounts of matter, according to new data from NASA’s Chandra X-ray Observatory.

The new findings may help astronomers understand how the largest black holes were able to grow so rapidly in the early universe.

It also suggests that some quasars are even more adept at eating up material than scientists previously were aware of.

Study leader Bin Luo, postdoctoral researcher working with Niel Brandt, professor of astronomy and astrophysics at Penn State, said:

“Even for famously prodigious consumers of material, these huge black holes appear to be dining at enormous rates, at least five to ten times faster than typical quasars.”

Astronomers have known for some time that supermassive black holes, with masses ranging from millions to billions of times the mass 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.””

Ravenous Donuts

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 donut shape that surrounds the inner part of the disk.

Co-author Jianfeng Wu of the Harvard-Smithsonian Center for Astrophysics, says:

“This picture fits with our data. If a quasar is embedded in a thick donut-shaped structure of gas and dust, the donut 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,” says Brandt.

The key 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.

Reference:

B. Luo, W. N. Brandt, P. B. Hall, Jianfeng Wu, S. F. Anderson, G. P. Garmire, R. R. Gibson, R. M. Plotkin, G. T. Richards, D. P. Schneider, O. Shemmer, Yue Shen
X-ray Insights into the Nature of PHL 1811 Analogs and Weak Emission-Line Quasars: Unification with a Geometrically Thick Accretion Disk?
arXiv:1503.02085 [astro-ph.GA]

Illustration by M. Weiss/CXC via Penn State