A violent, complex scene of colliding galaxy clusters

Jun 03, 2014
Colliding galaxy clusters MACS J0717+3745, more than 5 billion light-years from Earth. Background is Hubble Space Telescope image; blue is X-ray image from Chandra, and red is VLA radio image. Credit: Van Weeren, et al.; Bill Saxton, NRAO/AUI/NSF; NASA.

Astronomers using the Karl G. Jansky Very Large Array (VLA) and the Chandra X-Ray Observatory have produced a spectacular image revealing new details of violent collisions involving at least four clusters of galaxies. Combined with an earlier image from NASA's Hubble Space Telescope (HST), the new observations show a complex region more than 5 billion light-years from Earth where the collisions are triggering a host of phenomena that scientists still are working to understand.

The HST image forms the background of this composite, with the X-ray emission detected by Chandra in blue and radio emission seen by the VLA in red. The X-rays indicate hot, tenuous gas that pervades the region containing the . The large, oddly-shaped red feature at the center probably is a region where shocks caused by the collisions are accelerating particles that then interact with magnetic fields and emit the .

"The complex shape of this region is unique; we've never spotted anything like this before," said Reinout van Weeren, an Einstein Fellow at the Harvard-Smithsonian Center for Astrophysics. "The shape probably is the result of the multiple ongoing collisions," he added.

The new radio and X-ray observations are much more sensitive than previous ones, the scientists said. The combination of these images will make this region one of the best-studied examples of cluster-cluster collisions yet known, and can yield new insights on the complex interactions during cluster mergers. Together, the merging clusters are called MACS J0717+3745, which also is one of the HST Frontier Fields for which HST will produce the deepest observations ever. The scientists presented their findings to the American Astronomical Society's meeting in Boston, Mass.

The straight, elongated radio-emitting object is a foreground galaxy whose central black hole is accelerating jets of particles in two directions. The red object at bottom-left is a radio galaxy that probably is falling into the cluster.

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1 / 5 (2) Jun 03, 2014
Merger mania continues....Just replace the word 'merging' with the word 'diverging', and the word 'collisions' with 'divisions', and the article will then be understandable.
5 / 5 (3) Jun 03, 2014
"Just replace the word 'merging' with the word 'diverging'"

Why would you want to lie about what is observed. This massive cluster (~2x10^15 Msun) is actually composed of 4 subclusters, designated A, B, C & D. Of these, "B" is *observed* to be falling towards the cluster's center at ~3000 km/s. A 2009 spectroscopic study of the cluster revealed:

"...the galaxies associated with feature B are found to move through the cluster core at a very high relative radial velocity of over 3000 km s-1, close to the maximal velocity expected from infall from infinity."


But your advice is to lie about what is *observed* and say that subcluster B is receding (diverging) from the cluster. I get that observations are the opposite of what your predetermined sci-fi fantasy tells you (and based on no observations of this particular cluster whatsoever), but really there's no need to lie about it.
1 / 5 (3) Jun 03, 2014
One of four moving as hoped. All based on a likely incorrect assumption between red shift and actual speed. Merger mania continues. The interpretation is biased. Cool your dipolic jets. I am not lying. Just pointing out the observational bias, built into the system. Without this bias, one cannot get published. And once published, it becomes an almost biblical reference to be celebrated. It's the system of interpretation that distorts reality, and leads to fantasy models, like the Huge Bang.
5 / 5 (3) Jun 03, 2014
"One of four moving as hoped."

One of four moving (merging) as *observed*. We even see the results of this merger in X-rays (see previous link). Got observations that show any component rapidly moving away from this cluster?

I thought not.