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Composite near-infrared and X-ray image of the galaxy cluster CL J1449+0856

Composite near-infrared and X-ray image of the galaxy cluster CL J1449+0856


Date: 08 March 2011
Satellite: XMM-Newton
Depicts: Composite image of galaxy cluster CL J1449+0856
Copyright: ESA/ESO/Subaru/R. Gobat et al.

This image shows the X-ray emission (in purple) coming from the diffuse intra-cluster medium of the galaxy cluster CL J1449+0856 as detected by XMM-Newton.

The X-ray signal is superimposed onto a composite image of very long exposures taken at near-infrared wavelengths with ESO's Very Large Telescope in Chile and the Subaru telescope on Hawaii. Most of the objects visible in the field are very faint and distant galaxies: the galaxy cluster is visible as a clump of faint, red objects near the centre.

Located at a redshift z~2, CL J1449+0856 is the most distant mature cluster ever detected.

The cluster luminosity (L) is approximately 7 × 1043 erg/s in the soft X-ray energy range (0.1-2.4 keV), and corresponds to a temperature of 2 keV (about 23 million Kelvin) and an estimated mass of 5-8 × 1013 solar masses.

The region depicted above is about 100 arc minutes on a side.

Last Update: 1 September 2019
1-Jul-2022 16:51 UT

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