X-ray: NASA/CXC/UCDavis/F. Bouhrik et al.;
Optical:Legacy Survey/DECaLS/BASS/MzLS; Image Processing: NASA/CXC/SAO/P.
Edmonds and L. Frattare
Celebrate the New Year with the “Champagne Cluster,” a galaxy cluster seen
in this new image from NASA’s Chandra X-ray Observatory and optical telescopes.
Astronomers discovered this galaxy
cluster Dec. 31, 2020. The date, combined with the bubble-like appearance of
the galaxies and the superheated gas seen with Chandra observations
(represented in purple), inspired the scientists to nickname the galaxy cluster
the Champagne Cluster, a much easier-to-remember name than its official
designation of RM J130558.9+263048.4.
The new composite image shows that
the Champagne Cluster is actually two galaxy clusters in the process of merging
to form an even larger cluster. Multimillion-degree gas in galaxy clusters
usually takes on an approximately circular or moderately oval shape in images,
but in the Champagne Cluster it is more widely spread from top to bottom,
revealing the presence of the two colliding clusters. Two clumps of individual
galaxies making up the colliding clusters can be seen toward the top and bottom
of center. (The image has been rotated clockwise by 90 degrees so that North
points to the right.)
The hot gas outweighs the combined
mass in all of the hundred-plus individual galaxies in the newly forming
cluster. The clusters also contain even larger amounts of unseen dark matter,
the mysterious substance that pervades the universe.
In addition to the Chandra data,
this new image contains optical data from the Legacy Surveys (red, green, and
blue), which consists of three individual and complementary surveys from
various telescopes in Arizona and Chile.
The Champagne Cluster is a member
of a rare class of merging clusters, which includes the well-known Bullet
Cluster, where the hot gas in each cluster has collided and slowed down, and
there is a clear separation between the hot gas and the most massive galaxy in
each cluster.
By comparing the data with computer
simulations, astronomers came up with two possibilities for the history of the
Champagne Cluster. One is that the two clusters already collided with each
other over two billion years ago. After the collision the two clusters traveled
outward and then were pulled back toward each other by gravity, and are now
heading into a second collision. The other idea is that a single collision
occurred about 400 million years ago, and the two clusters are now traveling
away from each other after that collision. Researchers think further studies of
the Champagne Cluster can potentially teach them how dark matter reacts to a
high-speed collision.
A paper describing these results
recently appeared in The Astrophysical Journal and is available online. The authors of the paper are Faik Bouhrik, Rodrigo Stancioli, and David
Wittman, all from the University of California, Davis.
NASA’s Marshall Space Flight Center
in Huntsville, Alabama, manages the Chandra program. The Smithsonian
Astrophysical Observatory’s Chandra X-ray Center controls science operations
from Cambridge, Massachusetts, and flight operations from Burlington, Massachusetts.
Visual Description
This release features a composite
image of a galaxy cluster discovered on New Year’s Eve day, 2020.
The cluster appears here as a large
collection of brilliant white lights, each a distinct galaxy. A neon purple
cloud stretches across the cluster’s crowded core. Many of the hundred-plus
galaxies in the cluster are in two clumps of galaxies towards the top and
bottom of center. Some are encircled by a faint glowing haze, while a few
foreground stars gleam with diffraction spikes. Some of the smaller galaxies
are tinted blue, orange, or red, and some appear more oblong than round,
suggesting spiral shapes viewed edge-on.
The neon purple cloud sits at the
heart of the image, surrounding the most densely-packed part of the cluster.
This cloud, which spreads vertically across the cluster, is multimillion-degree
gas observed by Chandra. The two clumps of observable galaxies, and the spread
of superheated gas, reveal that the Champagne Cluster is in fact two clusters
in the process of colliding.
With the two clusters of sparkling light clinking together, and the auspicious discovery date, astronomers have dubbed the merged cosmic structure “The Champagne Cluster”.
Source: NASA's Chandra Rings in New Year With Champagne Cluster - NASA

