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'Death Star' Black Hole Fires At Neighboring Galaxy

Date:
December 18, 2007
Source:
Chandra X-ray Observatory
Summary:
A jet from a black hole at the center of a galaxy strikes the edge of another galaxy. This is the first time such an interaction has been found. The jet impacts the companion galaxy at its edge and is then disrupted and deflected, much like how a stream of water from a hose will splay out after hitting a wall at an angle. Each wavelength shows a different aspect of this system, known as 3C321. The Chandra X-ray image provides evidence that each galaxy contains a rapidly growing supermassive black hole at its center.
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FULL STORY

This composite image shows the jet from a black hole at the center of a galaxy striking the edge of another galaxy, the first time such an interaction has been found. In the image, data from several wavelengths have been combined. X-rays from Chandra (colored purple), optical and ultraviolet (UV) data from Hubble (red and orange), and radio emission from the Very Large Array (VLA) and MERLIN (blue) show how the jet from the main galaxy on the lower left is striking its companion galaxy to the upper right.
Credit: Credit: X-ray: NASA/CXC/CfA/D.Evans et al.; Optical/UV: NASA/STScI; Radio: NSF/VLA/CfA/D.Evans et al., STFC/JBO/MERLIN

A jet from a black hole at the center of a galaxy strikes the edge of another galaxy. This is the first time such an interaction has been found. The jet impacts the companion galaxy at its edge and is then disrupted and deflected, much like how a stream of water from a hose will splay out after hitting a wall at an angle.

Each wavelength shows a different aspect of this system, known as 3C321. The Chandra X-ray image provides evidence that each galaxy contains a rapidly growing supermassive black hole at its center. The glow from the stars in each galaxy can be detected from Hubble's optical light images (not shown).

A bright spot in the VLA and MERLIN radio image shows where the jet has struck the side of the galaxy - about 20,000 light years from the main galaxy - dissipating some of its energy. An even larger "hotspot" of radio emission detected by VLA reveals that the jet terminates much farther away from the galaxy, at a distance of about 850,000 light years away.

Large quantities of warm and hot gas could be detected in the vicinity of the galaxies, indicating the supermassive black holes in both galaxies have had a violent past. Faint emission from Chandra, Hubble and Spitzer, not shown in this image, indicate that the galaxies are orbiting in a clockwise direction, implying that the companion galaxy is swinging into the path of the jet.

Since the Chandra data shows that particle acceleration is still occurring in this hotspot, the jet must have struck the companion galaxy relatively recently, less than about a million years ago (i.e. less than the light travel time to the hotspot). This relatively short cosmic time frame makes this event a very rare phenomenon.

This "death star galaxy" will produce large amounts of high-energy radiation, which may cause severe damage to the atmospheres of any planets in the companion galaxy that lie in the path of the jet.

From the Earth we look down the barrel of jets from supermassive black holes, however these so-called "blazars" are at much safer distances of millions or billions of light years.


Story Source:

The above story is based on materials provided by Chandra X-ray Observatory. Note: Materials may be edited for content and length.


Cite This Page:

Chandra X-ray Observatory. "'Death Star' Black Hole Fires At Neighboring Galaxy." ScienceDaily. ScienceDaily, 18 December 2007. <www.sciencedaily.com/releases/2007/12/071218103611.htm>.
Chandra X-ray Observatory. (2007, December 18). 'Death Star' Black Hole Fires At Neighboring Galaxy. ScienceDaily. Retrieved April 26, 2015 from www.sciencedaily.com/releases/2007/12/071218103611.htm
Chandra X-ray Observatory. "'Death Star' Black Hole Fires At Neighboring Galaxy." ScienceDaily. www.sciencedaily.com/releases/2007/12/071218103611.htm (accessed April 26, 2015).

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