Abell 2744

Different Wavelengths in Abell 2744

Multi wavelength composite astronomical image using data from the Jansky Very Large Array, Chandra X-ray Observatory, and optical data from the VLT and Subaru Telescopes. Animated GIF cycles through the individual images (radio, X-ray, optical) of Abell 2744.

VLA image of Abell 2744

Abell 2744, Radio Only

Radio-only image of Abell 2744 region, showing radio-emitting features caused by subatomic particles accelerated to high speeds by the collisions of giant clusters of galaxies.

Before and after radio detection.
Comparison of NVSS, FIRST, and VLASS images.

VLASS Sharpens the View

The new VLA Sky Survey (VLASS) sharpens the view. Here is the same radio-emitting object as seen, from left to right, with the NRAO VLA Sky Survey (NVSS), the FIRST Survey, and the VLASS. The VLASS image, unlike the others, allows astronomers to positively identify the image as jets of material propelled outward from the center of a galaxy that also is seen in the visible-light Sloan Digital Sky Survey. Technical data: NVSS image at 1.4 GHz in VLA’s D configuration; FIRST image at 1.4 GHz in B configuration; VLASS image at 3 GHz in B configuration.

Radio-emitting mini-halo in Perseus Cluster

VLA Gives New Insight Into Galaxy Cluster’s Spectacular “Mini-Halo”

Astronomers using the National Science Foundation’s Karl G. Jansky Very Large Array (VLA) have discovered new details that are helping them decipher the mystery of how giant radio-emitting structures are formed at the center of a cluster of galaxies. The scientists studied a cluster of thousands of galaxies more than 250 million light-years from Earth, named the Perseus Cluster after the constellation in which it appears. Embedded within the center, the Perseus Cluster hosts a pool of superfast particles that emit radio waves, creating a radio structure known as a “mini-halo.” Mini-haloes have been found in about 30 galaxy clusters, but the halo in the Perseus Cluster is the largest known, about 1.3 million light-years in diameter, or 10 times the size of our Milky Way Galaxy. Radio emission in red; optical in white.

1989 and 2015 images, with newly-discovered object seen and not seen.