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Survivor black holes may be mid-sized

Researchers have found signatures in X-ray data of two mid-sized black holes in the starburst galaxy M82.
Provided by the Chandra X-ray Center, Cambridge, Massachusetts
M82
Composite image of the nearby starburst galaxy M82.
X-ray: NASA/CXC/Tsinghua Univ./H. Feng et al.
April 30, 2010
New evidence from NASA's Chandra X-ray Observatory and ESA's XMM-Newton strengthens the case that two mid-sized black holes exist close to the center of a nearby starburst galaxy. These survivor black holes avoided falling into the center of the galaxy and could be examples of the seeds required for the growth of supermassive black holes in galaxies, including the one in the Milky Way.

For several decades, scientists have had strong evidence for two distinct classes of black holes — the stellar-mass variety with masses about 10 times that of the Sun and the supermassive ones located at the center of galaxies that range from hundreds of thousands to billions of solar masses.

But a mystery has remained: What about black holes that are in between? Evidence for these objects has remained controversial, and until now there were no strong claims of more than one such black hole in a single galaxy. Recently, a team of researchers has found signatures in X-ray data of two mid-sized black holes in the starburst galaxy M82, located 12 million light-years from Earth.

"This is the first time that good evidence for two mid-sized black holes has been found in one galaxy," said Hua Feng of the Tsinghua University in China. "Their location near the center of the galaxy might provide clues about the origin of the universe's largest black holes — supermassive black holes found in the centers of most galaxies."

One possible mechanism for the formation of supermassive black holes involves a chain reaction of collisions of stars in compact star clusters that results in the buildup of extremely massive stars, which then collapse to form intermediate-mass black holes. The star clusters then sink to the center of the galaxy where the intermediate-mass black holes merge to form a supermassive black hole.

In this case, clusters that were not massive enough or close enough to the center of the galaxy to fall in would survive, as would any black holes they contain.

"We can't say whether this process actually occurred in M82, but we do know that both of these possible mid-sized black holes are located in or near star clusters," said Phil Kaaret from the University of Iowa. "Also, M82 is the nearest place to us where the conditions are similar to those in the early universe with lots of stars forming."

The evidence for these two survivor black holes comes from how their X-ray emission varies over time and analysis of their X-ray brightness and spectra — the distribution of X-rays with energy.

Chandra and XMM-Newton data show that the X-ray emission for one of these objects changes in a distinctive manner similar to stellar-mass black holes found in the Milky Way. Using this information and theoretical models, the team estimated that this black hole's mass is between 12,000 and 43,000 times the mass of the Sun. This mass is large enough for the black hole to generate copious X-rays by pulling gas directly from its surroundings rather than from a binary companion like with stellar-mass black holes.

The black hole is located at a projected distance of 290 light-years from the center of M82. The scientists estimate that at this close distance if the black hole was born at the same time as the galaxy and its mass was more than about 30,000 solar masses, it would have been pulled into the center of the galaxy. That is, it may have just escaped falling into the supermassive black hole that is presumably located in the center of M82.

Both Chandra and XMM-Newton observed the second object, located 600 light-years in projection away from the center of M82. During X-ray outbursts, periodic and random variations normally present in the X-ray emission disappear, a strong indication that a disk of hot gas dominates the X-ray emission. A detailed fit of the X-ray data indicates that the disk extends all the way to the innermost stable orbit around the black hole. Similar behavior has been seen from stellar-mass black holes in our galaxy, but this is the first likely detection in an intermediate-mass black hole candidate.

The radius of the innermost stable orbit depends only on the mass and spin of the black hole. The best model for the X-ray emission implies a rapidly spinning black hole with mass in the range of 200 to 800 times the mass of the Sun. The mass agrees with theoretical estimates for a black hole created in a star cluster by runaway collisions of stars.

"This result is one of the strongest pieces of evidence to date for the existence of an intermediate-mass black hole," said Feng. "This looks just like well-studied examples of stellar-mass black holes, except for being more than 20 times as massive."
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