Black Hole Gets Jerked Around -- Twice

Jul 21, 2010
This version of the composite X-ray and radio image is labeled to show the different cavities identified by the scientists. Credit: X-ray: NASA/CXC/UMD/Hodges-Kluck et al. Radio: NSF/AUI/NRAO/VLA/UMD/Hodges-Kluck et al.

( -- Scientists have found evidence that a giant black hole has been jerked around twice, causing its spin axis to point in a different direction from before. This discovery, made with new data from NASA's Chandra X-ray Observatory, might explain several mysterious-looking objects found throughout the Universe.

The axis of the spinning black hole is thought to have moved, but not the black hole itself, so this result differs from recently published work on recoiling .

"We think this is the best evidence ever seen for a black hole having been jerked around like this," said Edmund Hodges-Kluck of the University of Maryland. "We're not exactly sure what caused this behavior, but it was probably triggered by a collision between two galaxies."

A team of astronomers used Chandra for a long observation of a galaxy known as 4C +00.58, which is located about 780 million light years from Earth. Like most galaxies, 4C +00.58 contains a at its center, but this one is actively pulling in copious quantities of gas. Gas swirling toward the black hole forms a disk around the black hole. Twisted magnetic fields in the disk generate strong electromagnetic forces that propel some of the gas away from the disk at high speed, producing radio jets.

A radio image of this galaxy shows a bright pair of jets pointing from left to right and a fainter, more distant line of radio emission running in a different direction. More specifically, 4C +00.58 belongs to a class of "X-shaped" galaxies, so called because of the outline of their radio emission.

The new Chandra data have allowed astronomers to determine what may be happening in this system, and perhaps in others like it. The X-ray image reveals four different cavities around the black hole. These cavities come in pairs: one in the top-right and bottom-left, and another in the top-left and bottom-right.

When combined with the orientation of the , the complicated geometry revealed in the Chandra image may tell the story of what happened to this supermassive black hole and the galaxy it inhabits.

The close-up view in the inset shows a composite image of the galaxy 4C +00.58 in X-rays from Chandra (gold) and radio waves from the Very Large Array (blue). New data suggest the giant black hole has been flipped around, causing its spin axis to point in a different direction from before. The deep Chandra X-ray image shows hot gas in and around 4C +00.58 and reveals four different cavities -- regions of lower than average X-ray emission -- around the black hole. The X-ray data when combined with the radio information suggests that collisions with other galaxies may have caused the black hole to shift the direction it was spinning. Credit: NASA/CXC/UMD/Hodges-Kluck et al.

"We think that this black hole has quite a history," said Christopher Reynolds of the University of Maryland in College Park. "Not once, but twice, something has caused this black hole to change its spin axis."

According to the scenario presented by Hodges-Kluck and his colleagues, the spin axis of the black hole ran along a diagonal line from top-right to bottom-left. After a collision with a smaller galaxy, a jet powered by the black hole ignited, blowing away gas to form cavities in the hot gas to the top-right and bottom-left. Since the gas falling onto the black hole was not aligned with the spin of the black hole, the spin axis of the black hole rapidly changed direction, and the jets then pointed in a roughly top-left to bottom-right direction, creating cavities in the hot gas and radio emission in this direction.

Then, either a merging of the two central from the colliding galaxies, or more gas falling onto the black hole, caused the spin axis to jerk around to its present direction, roughly left to right. These types of changes in the angle of the spin of a supermassive black hole have previously been suggested to explain X-shaped radio galaxies, but no convincing case has been made for any individual object.

"If we're right, our work shows that jets and cavities are like cosmic fossils that help trace the merger history of an active supermassive black hole and the galaxy it lives in," said Hodges-Kluck. "If even a fraction of X-shaped radio are produced by such "spin-flips", then their frequency may be important for estimating the detection rates with gravitational radiation missions."

Explore further: Toothpaste fluorine formed in stars

More information: These results appeared in a recent issue of The Astrophysical Journal Letters.

Related Stories

Black Hole Pumps Iron

Sep 14, 2009

( -- This composite image of the Hydra A galaxy cluster shows 10-million- degree gas observed by Chandra in blue and jets of radio emission observed by the Very Large Array in pink. Optical data ...

An Intriguing, Glowing Galaxy

May 14, 2009

A supermassive black hole may be responsible for the glowing appearance of galaxy 3C 305, located about 600 million light years away in the constellation Draco. Composite data from NASA’s Chandra X-ray Observatory ...

Chandra data reveal rapidly whirling black holes

Jan 10, 2008

A new study using results from NASA's Chandra X-ray Observatory provides one of the best pieces of evidence yet that many supermassive black holes are spinning extremely rapidly. The whirling of these giant ...

Image: Black Hole Blows Big Bubble

Jul 12, 2010

This composite image shows a powerful microquasar produced by a black hole in the outskirts of the nearby (12.7 million light years) galaxy NGC 7793. The large image contains data from the Chandra X-ray Observatory ...

Supermassive black hole is thrown out of galaxy

May 11, 2010

( -- Undergraduate student Marianne Heida of the University of Utrecht has found what appears to be a supermassive black hole leaving its home galaxy at high speed. As part of an international ...

Recommended for you

Toothpaste fluorine formed in stars

2 hours ago

The fluorine that is found in products such as toothpaste was likely formed billions of years ago in now dead stars of the same type as our sun. This has been shown by astronomers at Lund University in Sweden, ...

Swirling electrons in the whirlpool galaxy

22 hours ago

The whirlpool galaxy Messier 51 (M51) is seen from a distance of approximately 30 million light years. This galaxy appears almost face-on and displays a beautiful system of spiral arms.

A spectacular landscape of star formation

Aug 20, 2014

This image, captured by the Wide Field Imager at ESO's La Silla Observatory in Chile, shows two dramatic star formation regions in the Milky Way. The first, on the left, is dominated by the star cluster NGC ...

Exoplanet measured with remarkable precision

Aug 19, 2014

Barely 30 years ago, the only planets astronomers had found were located right here in our own solar system. The Milky Way is chock-full of stars, millions of them similar to our own sun. Yet the tally ...

User comments : 4

Adjust slider to filter visible comments by rank

Display comments: newest first

3.7 / 5 (6) Jul 21, 2010
No one blathering on about aether or plasma. How refreshing.
2 / 5 (4) Jul 21, 2010
"No one blathering on about aether or plasma. How refreshing."

A bunch of wild conjecture without foundation in empirical evidence, or plasma. I think I know who is being jerked around...
1.5 / 5 (2) Jul 21, 2010
My best guess is that we have two black holes in a binary system... Should produce the same effect!
4.5 / 5 (2) Jul 22, 2010
X-shaped radio galaxies have gained a lot of attention since their discovery in the early 1990s and the later realization that black hole mergers could be the culprit: http://en.wikiped...o_galaxy

"My best guess is that we have two black holes in a binary system..."

Evidence shows that only one black hole is present, so they've already merged(in the likely case of a binary BH merger), but the jets from the pre-merger phase remain along with the current pair of jets.