Abell 1033: To boldly go into colliding galaxy clusters

Abell 1033: To boldly go into colliding galaxy clusters
Composite image. Credit: Chandra X-ray Center

Hidden in a distant galaxy cluster collision are wisps of gas resembling the starship Enterprise—an iconic spaceship from the "Star Trek" franchise.

Galaxy clusters—cosmic structures containing hundreds or even thousands of galaxies—are the largest objects in the Universe held together by gravity. Multi-million-degree gas fills the space in between the individual galaxies. The mass of the hot gas is about six times greater than that of all the combined. This superheated gas is invisible to optical telescopes, but shines brightly in X-rays, so an X-ray telescope like NASA's Chandra X-ray Observatory is required to study it.

By combining X-rays with other types of light, such as , a more complete picture of these important cosmic objects can be obtained. A new composite image of the galaxy cluster Abell 1033, including X-rays from Chandra (purple) and radio from the Low-Frequency Array (LOFAR) network in the Netherlands (blue), does just that. Optical emission from the Sloan Digital Sky Survey is also shown. The galaxy cluster is located about 1.6 billion light years from Earth.

Using X-ray and radio data, scientists have determined that Abell 1033 is actually two in the process of colliding. This extraordinarily energetic event, happening from the top to the bottom in the image, has produced turbulence and shock waves, similar to sonic booms produced by a plane moving faster than the speed of sound.

Abell 1033: To boldly go into colliding galaxy clusters
X-ray wavelength. Credit: Chandra X-ray Center

In Abell 1033, the collision has interacted with another energetic cosmic process—the production of jets of high-speed particles by matter spiraling into a , in this case one located in a galaxy in one of the clusters. These jets are revealed by radio emission to the left and right sides of the image. The radio emission is produced by spiraling around magnetic field lines, a process called synchrotron emission.

The electrons in the jets are traveling at very close to the speed of light. As the galaxy and its black hole moved toward the lower part of the image, the jet on the right slowed down as it crashed into hot gas in the other galaxy cluster. The jet on the left did not slow down because it encountered much less hot gas, giving a warped appearance for the jets, rather than the straight line that is typically seen.

This image of Abell 1033 also provides an example of "pareidolia", a psychological phenomenon where familiar shapes and patterns are seen in otherwise random data. In Abell 1033, the structures in the data create an uncanny resemblance to many of the depictions of the fictional Starship Enterprise from Star Trek.

Abell 1033: To boldly go into colliding galaxy clusters
Optical wavelength. Credit: Chandra X-ray Center

In terms of astrophysical research, a detailed study of the image shows that the energy of the electrons in the "saucer section" and neck of the starship-shaped radio emission in Abell 1033 is higher than that found in the stardrive section towards the lower left (see labels). This suggests that the electrons have been reenergized, presumably when the jets interact with turbulence or shock waves in the hot gas. The energetic electrons producing the radio emission will normally lose substantial amounts of energy over tens to hundreds of millions of years as they radiate. The radio emission would then become undetectable. However, the vastly extended radio emission observed in Abell 1033, extending over about 500,000 light years, implies that energetic electrons are present in larger quantities and with higher energies than previously thought. One idea is that the electrons have been given a further boost in energy by extra bouts of shocks and turbulence.

Abell 1033: To boldly go into colliding galaxy clusters
Radio emission visualization. Credit: Chandra X-ray Center

Other sources of radio emission in the image besides the starship-shaped object are the shorter jets from another galaxy (labeled "short ") and a "radio phoenix" consisting of a cloud of electrons that faded in radio emission but was then reenergized when shock waves compressed the cloud. This caused the cloud to once again shine at frequencies, as we reported back in 2015.

The team who made this study will use observations with Chandra and LOFAR to look for further examples of colliding galaxy clusters with warped , to further their understanding of these energetic objects.

A paper describing this result was published in the October 4th, 2017 issue of Science Advances.

Abell 1033: To boldly go into colliding galaxy clusters
USS Enterprise NCC 1701. Credit: Smithsonian National Air & Space Museum

Explore further

Chandra data suggest giant collision triggered 'radio phoenix'

More information: Francesco de Gasperin et al. Gentle reenergization of electrons in merging galaxy clusters, Science Advances (2017). DOI: 10.1126/sciadv.1701634
Journal information: Science Advances

Citation: Abell 1033: To boldly go into colliding galaxy clusters (2018, November 16) retrieved 14 December 2019 from https://phys.org/news/2018-11-abell-boldly-colliding-galaxy-clusters.html
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