Multiwavelength image of the 'Toothbrush' galaxy cluster

Multiwavelength image of the "Toothbrush" galaxy cluster
A multiwavelength false-color image of the "Toothbrush" cluster of galaxies, 1RXS J0603.3+4214. The intensity in red shows the radio emission, blue is X -ray, and the background color composite is optical emission. Astronomers studying the cluster with new radio observations combined with other wavelengths have been able to confirm the galaxy merger scenario and estimate the magnetic field strength in the shocks. Credit: van Weeren et al.

Most galaxies lie in clusters containing from a few to thousands of objects. Our Milky Way, for example, belongs to a cluster of about fifty galaxies called the Local Group whose other large member is the Andromeda galaxy about 2.3 million light-years away. Clusters are the most massive gravitationally bound objects in the universe and form (according to current ideas) in a "bottoms-up" fashion with smaller structures developing first and larger groupings assembling later in cosmic history. Dark matter plays an important role in this growth process.

Exactly how they grow, however, appears to depend on several competing physical processes including the behavior of the intracluster gas. There is more mass in this gas than there is in all the stars of a 's , and the gas can have a temperature of ten million kelvin or even higher. As a result, the gas plays an important role in the cluster's evolution. The hot intracluster gas contains rapidly moving charged particles that radiate strongly at radio wavelengths, sometimes revealing long filamentary structures.

The "Toothbrush" galaxy cluster, 1RXS J0603.3+4214, hosts three of these radio structures as well as a large halo. The most prominent radio feature extends over more than six million light years, with three distinct components that resemble the brush and handle of a toothbrush. The handle is particularly enigmatic because, besides being large and very straight, it is off center from the axis of the cluster. The halo is thought to result from turbulence produced by the of galaxies, although some other possibilities have been suggested.

CfA astronomers Reinout van Weeren, Bill Forman, Felipe Andrade-Santos, Ralph Kraft, and Christine Jones and their colleagues used the Very Large Array (VLA) facility to observe the relativistic particles in the cluster with precise, sensitive radio imaging, which they compared with Chandra X-ray and other datasets. In the radio, the Toothbrush has a very narrow ridge, created by a huge shock resulting from the merger, and at least thirty-two previously undetected compact sources. The halo's and X-ray morphologies are very similar and lend support to the merger scenario. Astronomers are also able to estimate the strength of the magnetic field, and combined with other results, use it to conclude that the merger scenario is most suitable.


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More information: "Deep VLA Observations of the Cluster 1RXS J0603.3+4214 in the Frequency Range 1-2 GHz," K. Rajpurohit, M. Hoeft, R. J. van Weeren, L. Rudnick, H. J. A. R ottgering, W. R. Forman, M. Bruggen, J. H. Croston, F. Andrade-Santos, W. A. Dawson, H. T. Intema, R. P. Kraft, C. Jones, and M. James Jee, ApJ 2017 (in press). lanl.arxiv.org/abs/1712.01327
Citation: Multiwavelength image of the 'Toothbrush' galaxy cluster (2017, December 27) retrieved 19 July 2019 from https://phys.org/news/2017-12-multiwavelength-image-toothbrush-galaxy-cluster.html
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Dec 27, 2017
\"... and form (according to current ideas) in a "bottoms-up" fashion...\"

Lots of people are formed this way too, how about that?

Also hoping to read about the role of the AETHER on cluster growth later today, please don't dissappoint.

Dec 27, 2017
IU, sorry buddy. But I ain't gonna mention that ridiculous notion of crackedpotty charlatans.

I admire the effort this article's research team has put into collecting verified data. Without adding, as of yet unconfirmed evidence, to conflate speculations as conclusive proof of one hypothesis or another.

This research program is an excellent example of why developing new tools enables the progress of science.

Jan 03, 2018
cue the sad trombone -

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