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The Chandra image of NGC 6240, a butterfly-shaped galaxy that is the product of the collision of two smaller galaxies, revealed that the central region of the galaxy (inset) contains not one, but two active giant black holes.


An artist's conception shows a black hole surrounded by a disk of hot gas, and a large doughnut or torus of cooler gas and dust. The light blue ring on the back of the torus is due to the fluorescence of iron atoms excited by X-rays from the hot gas disk.
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By Robert Roy Britt
Senior Science Writer
posted: 12:15 pm ET
19 November 2002

For the first time, scientists have proof of that a pair of supermassive black holes exist together in the same galaxy, thanks to data from NASA's Chandra X-ray Observatory

A pair of gargantuan black holes have been found to inhabit the same galaxy and will eventually merge with a violence that will slingshot stars out of the galaxys center and unleash a torrent of radiation and gravitational energy.

The discovery is the first proof that one galaxy can contain two supermassive black holes, astronomers said today at a NASA press conference. The work also adds to other theoretical suggestions that black holes can in fact merge.

Researchers have known that the galaxy known as NGC 6240 has two bright spots, called nuclei, near its center, based on observations with radio, infrared and optical telescopes. Since the central region of the galaxy is shrouded in dust, however, it cant be observed in much detail.

To investigate the pair, scientists pointed the Chandra X-ray Observatory at it. X-rays penetrate dust.

"With Chandra, we hoped to determine which one, if either, of the nuclei was an active supermassive black hole," said Stefanie Komossa of the Max Planck Institute for Extraterrestrial Physics. "Much to our surprise, we found that both were active black holes."

Active black holes are those that are actively consuming matter. Astronomers detect them because some of the incoming matter is not consumed, but rather is converted to energy in a frenetic environment of high-speed travel. The stuff is shot out as X-rays, other radiation and superheated matter called plasma.

Our own Milky Way harbors a supermassive black hole weighing as much as 2.6 million Suns. It is not, however, very active. A study earlier this year suggested that black hole mergers could serve as an on-off switch for the input and output of a black hole.

The collision

The galaxy Komossa and her colleagues examined is about 400 million light-years away, close by astronomical standards in a universe that spans more than 12 billion light years. The two black holes are about 3,000 light-years apart and closing. Each used to anchor a separate galaxy, but the two galaxies begin merging about 30 million years ago, astronomers estimate.

When galaxies merge, individual stars are typically not affected, theorists believe. But with two black holes colliding, thing get a little more chaotic. SPACE.com asked Komossa what will happen.

For now, the two black holes do not feel each others gravity directly, Komossa explained. Stars are unaffected because they are so widely separated. But the overall centers of the two galaxies are interacting gravitationally.

As the black holes draw closer, some stars will begin to feel the effect.

"Individual stars which approach the binary black hole closely are accelerated and finally ejected from the center of the galaxy," she said. "The energy is extracted from the orbital energy of the black hole binary."

The mechanism is the same slingshot effect NASA uses to sent spacecraft around a planet, robbing a tiny bit of the planets energy to give the craft a speed boost and fling it a more distant planet.

Making waves

When the black holes get as close as 1 light-year apart, they will begin to merge.

"They are now spiraling towards each other," Komossa said of that future event. "The final merging of the black holes, to form a single one of larger mass, will be accompanied by an enormous burst of gravitational waves."

These waves will spread through the universe, causing ripples in the fabric of space that astronomers would be able to detect as tiny changes in distance between two points.

"This is the first time that we see a binary black hole in action, the smoking gun for something which will become a major gravitational wave burst in the future," said Guenther Hasinger, another Max Planck researcher involved in the work.

Meanwhile, theres more to the merger. During the final stages, more and more gas rains down on the two black holes.

Komossa: "The gas will heat itself up in the process, and start to emit huge amounts of radiation, strongly increasing the luminosity of the nucleus of the galaxy, outshining the whole galaxy in its brightness by a large factor. The strong radiation field will start to destroy the dust in the environment of the nucleus, giving an outside observer an even clearer view on the nucleus of the galaxy.

"The powerful radiation will also hinder part of the infalling matter to actually reach the black holes horizon and disappear within the black hole; instead the material will be driven out again by strong radiation pressure, and huge outflows or jets may built up."

When all is said and done, few stars are likely to remain in the vicinity of the merged and more massive black hole.

One of many

Komossa said the new findings are indirect evidence that black holes must be in all states of merging around the universe.

She points out that NGC 6240 is relatively nearby, making the new and finely detailed observations possible. Astronomers have seen evidence for active black holes many billions of light years distant.

"The fact that we do see a binary black hole in this galaxy strongly suggests that there are many more out there," she said.

Other studies have shown that several gravitational wave event occur every year. A planned space detector called LISA (Laser Interferometer Space Antenna) would search for them.

 

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