A Super Galactic Discovery
NASA's Chandra X-ray Observatory spotted the two black holes in the galaxy NGC 6240. The observatory was able to "see" them because the black holes are surrounded by hot swirling vortices of matter called accretion disks. Such disks are strong sources of x-rays.
Above: An artist's concept of two black holes (surrounded by glowing hot accretion disks) about to merge. [see the animation]
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At a distance of about 400 million light-years, NGC 6240 is a prime example of a starburst galaxy--that is, a massive galaxy in which stars are forming at an exceptionally rapid rate due to a recent collision and subsequent merger of two smaller galaxies. Because of the large amount of dust and gas in such galaxies, it is difficult to peer deep into their central regions. Optical, radio, and infrared observations had previously revealed two bright nuclei, but their nature was a mystery.
X-rays, however, can penetrate the veil of gas and dust. "With Chandra, we hoped to determine which one, if either, of the nuclei was an active supermassive black hole," said Stefanie Komossa, also of the Max Planck Institute, lead author of the paper on NGC 6240. "Much to our surprise, we found that both were active black holes!"
"The detection of a binary black hole supports the idea that black holes can grow to enormous masses in the centers of galaxies by merging with other black holes," said Komossa. "This is important for understanding how galaxies form and evolve," she said.
Over the course of the next few hundred million years, the two black holes in NGC 6240, which are about 3000 light-years apart, will drift toward one another and merge to form an even larger supermassive black hole. Toward the end of this process an enormous burst of gravitational waves will be produced.
These gravitational waves will spread through the universe and produce ripples in the fabric of space, which would appear as minute changes in the distance between any two points. NASA's planned space-based detector, LISA (Laser Interferometer Space Antenna), will search for gravitational waves from massive black-hole mergers. These events are estimated to occur several times each year in the observable universe.
"This is the first time we see a binary black hole in action, the smoking gun for something that will become a major gravitational wave burst in the future," said Hasinger.
Chandra X-Ray Observatory -- This all-around site includes material for the press, for educators, and astronomy enthusiasts.
Max Planck Institute for Extraterrestrial Physics -- this is where Guenther Hasinger and Stefanie Komossa work.
Credits: Chandra observed NGC 6240 for 10.3 hours with the Advanced CCD Imaging Spectrometer (ACIS). Other members of the team are Vadim Burwitz and Peter Predehl of the Max Planck Institute, Jelle Kaastra of the Space Research Organization Netherlands and Yasushi Ikebe of the University of Maryland in Baltimore. NASA's Marshall Space Flight Center in Huntsville, Ala., manages the Chandra program for the Office of Space Science, Washington, and TRW, Inc., Redondo Beach, Calif., is the prime contractor for the spacecraft. The Smithsonian's Chandra X-ray Center controls science and flight operations from Cambridge, Mass.
X-ray Astronomy Field Guide: Black Holes -- find out more about stellar, mid-range, and supermassive black holes.
A Mystery in the Galactic Center -- (Science@NASA) Astronomers have learned that the center of our Milky Way galaxy harbors a long-sought black hole. But the finding has raised even more questions than before.
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