Astronomers Identify a New Mid-Size Black Hole

Credit: European Southern Observatory

A team led by astronomers at the University of Maryland and NASA’s Goddard Space Flight Center has found evidence for a new intermediate-mass black hole about 5,000 times the mass of the sun. The discovery adds one more candidate to the list of potential medium-sized black holes, while strengthening the case that these objects do exist. The team reported its findings in the September 21, 2015 online edition of Astrophysical Journal Letters.

The result follows up on a similar finding by some of the same scientists, using the same technique, published in August 2014. While the previous study accurately measured a black hole weighing 400 times the mass of the sun using data from NASA’s Rossi X-ray Timing Explorer (RXTE) satellite, the current study used data from the European Space Agency’s XMM-Newton satellite.

“This result provides support to the idea that black holes exist on all size scales. When you describe something for the first time, there is always some doubt,” said lead author Dheeraj Pasham, a postdoctoral associate at the Joint Space-Science Institute, a research partnership between UMD’s Departments of Astronomy and Physics and NASA Goddard. “Identifying a second candidate with a different instrument puts weight behind both findings and gives us confidence in our technique.”

The new intermediate-mass black hole candidate, known as NGC1313X-1, is classified as an ultraluminous X-ray source, and as such is among the brightest X-ray sources in the nearby universe. It has proven hard to explain exactly why ultraluminous X-ray sources are so bright, however. Some astronomers suspect that they are intermediate-mass black holes actively drawing in matter, producing massive amounts of friction and X-ray radiation in the process.

Against this backdrop of haphazard X-ray fireworks created by NGC1313X-1, Pasham and his colleagues identified two repeating flares, each flashing at an unusually steady frequency. One flashed about 27.6 times per minute and the other about 17.4 times per minute. Comparing these two rates yields a nearly perfect 3:2 ratio. Pasham and his colleagues also found this 3:2 ratio in M82X-1, the black hole they identified in August 2014, although the overall frequency of flashing was much higher in M82X-1.

Although astronomers are not yet sure what causes these steady flashes, the presence of a clockwork 3:2 ratio appears to be a common feature of stellar mass black holes and possibly intermediate-mass black holes as well. The flashes are most likely caused by activity close to the black hole, where extreme gravity keeps all surrounding matter on a very tight leash, Pasham said.

The 3:2 ratios can also provide an accurate measure of a black hole’s mass. Smaller black holes will flash at a higher frequency, while larger black holes will flash less often.

“To make an analogy with acoustic instruments, if we imagine that stellar mass black holes are the violin and supermassive black holes are the double bass, then intermediate-mass black holes are the violoncello,” said co-author Francesco Tombesi, an assistant research scientist in UMD’s Department of Astronomy who has a joint appointment at NASA Goddard via the Center for Research and Exploration in Space Science and Technology.

Pasham and Tombesi hope that identifying ultraluminous X-ray sources that exhibit the key 3:2 flashing ratio will yield many more intermediate-mass black hole candidates in the near future.

“Our method is purely empirical, it’s not reliant on models. That’s why it’s so strong,” Pasham explained. “We don’t know what causes these oscillations, but they appear to be reliable, at least in stellar mass black holes.”

NASA plans to launch a new X-ray telescope, the Neutron Star Interior Composition Explorer (NICER), in 2016. Pasham has already identified several potential intermediate-mass black hole candidates that he hopes to explore with NICER.

“Observing time is at a premium, so you need to build a case with an established method and a list of candidates the method can apply to,” Pasham explained. “With this result, we are in a good position to move forward and make more exciting discoveries.”

In addition to Pasham and Tombesi, UMD-affiliated co-authors include Astronomy Adjunct Assistant Professor Bradley Cenko and Astronomy Professor Richard Mushotzky.

Contacts and sources:
Matthew Wright