chandra_499 December 1st, 2010
Credit: X-ray: NASA/CXC/Rutgers/J.Hughes et al, Optical: ESO/VLT/Pontificia Universidad. Catolica de Chile/L.Infante & SOAR (MSU/NOAO/UNC/CNPq-Brazil)/Rutgers/F.Menanteau, IR: NASA/JPL/Rutgers/F.Menanteau
This galaxy cluster, which has been nicknamed "El Gordo" for the "big" or "fat" one in Spanish, is a remarkable object. Found in the distant Universe by Chandra and the Atacama Cosmology Telescope, El Gordo appears to be the most massive, the hottest, and gives off the most X-rays of any known cluster at its distance or beyond. In this composite image of El Gordo, X-rays are blue, optical data from the Very Large Telescope are red, green, and blue, and infrared emission from Spitzer is red. The comet-like shape of the X-rays, along with optical data, show that El Gordo is actually the site of a collision between two galaxy clusters, similar to the well-known Bullet Cluster.
Provider: Chandra X-ray Observatory
Image Source: http://chandra.harvard.edu/photo/2012/elgordo/
Curator: Chandra X-ray Observatory, Cambridge, MA, USA
Image Use Policy: http://chandra.harvard.edu/photo/image_use.html
Telescope | Spectral Band | Wavelength | |
---|---|---|---|
Chandra (ACIS) | X-ray (X-ray) | 826.7 pm | |
SOAR (SOI) | Optical (R-band) | 616.5 nm | |
SOAR (SOI) | Optical (I-band) | 748.1 nm | |
SOAR (SOI) | Optical (Z-band) | 893.1 nm | |
VLT (FORS2) | Optical (R-band) | 616.5 nm | |
VLT (FORS2) | Optical (I-band) | 748.1 nm | |
VLT (FORS2) | Optical (Z-band) | 893.1 nm | |
Spitzer (IRAC) | Infrared (Near-IR) | 3.6 µm | |
Spitzer (IRAC) | Infrared (Near-IR) | 4.5 µm | |
Detailed color mapping information coming soon...
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