Decam Reveals Hidden Cluster Light in Galaxy Cluster Abell 3667

The glow within the cluster is the soft luminosity of stars that have been stripped from their galaxy amidst the layers of galaxy clusters.



Abell 3667 is depicted in this Decam image. Image credits: CTIO/NOIRLAB/NSF/AURA/ANTHONY ENGLERT, Brown University/TA Rector, Noirlab/M. Zamani & D of University of Alaska Anchorage & NSF. De Martin, NSF’s Noirlab.

Galaxy clusters comprise thousands of galaxies, varying widely in age, shape, and size.

Typically, they have a mass about 10 billion times that of the Sun.

Historically, galactic clusters were regarded as the largest structures in the universe, spanning hundreds of millions of light-years and including numerous galactic clusters and groups, until superclusters were discovered in the 1980s.

Nonetheless, galaxy clusters still hold the title of the largest gravitationally bound structure in the universe.

“The study of galaxy clusters not only informs us about the formation of the universe, but it also places constraints on the characteristics of dark matter,” stated Brown University astronomer Anthony Englat and his team.

One significant clue astronomers seek to grasp the history of galactic clusters is the light within the cluster. This faint glow is emitted by stars that have been stripped from their original galaxy due to the immense gravitational forces of the forming galaxy cluster.

These stars provide evidence of past galactic interactions, although most current telescopes and cameras face challenges in detecting them.

The subtle intra-cluster light from the galaxy cluster Abel 3667 shines vividly in new images created from a total of 28 hours of observation at 570 megapixels using the Dark Energy Camera (Decam) at NSF’s M. Blanco 4-M Telescope, a program of NSF’s Noirlab at Cerro Tololo Inter-American Observatory.

“Abell 3667 is located over 700 million light-years away from us,” the astronomer mentioned.

“Most of the faint light sources in this image are distant galaxies, not foreground stars from our own Milky Way.”

“In Abell 3667, two small galaxy clusters are currently merging, as evidenced by the luminous bridge (yellow) of stars extending toward the center of this image.”

“This bridge is formed from material stripped off from the merging galaxies, forming one massive conglomerate known as the brightest cluster galaxy.”

“Not only does this sparkling sky encompass distant galaxies, but it also highlights faint foreground features due to the prolonged exposure.”

“The Milky Way’s hair follicles, or integrated flux nebula, consist of faint clouds of interstellar dust that appear as soft bluish chains crossing the image.”

“These structures are patches of dust that are illuminated by the light of the stars within our own galaxy.”

“They present as diffuse, filamentous formations that can span extensive areas of the sky.”

Survey results will be published in the Astrophysics Journal Letter.

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Anthony M. Engrat et al. 2025. Announcing optical bridges in Abel 3667 in-cluster light: LSST precursor data. apjl 989, L2; doi: 10.3847/2041-8213/ade8f1

Source: www.sci.news

DECam captures close-up of the Antria galaxy cluster

The Antria Galaxy Cluster is a group of at least 230 galaxies brought together by gravity. This galaxy cluster is rare. Unlike most other galaxy clusters, there appears to be no dominant galaxy within it.


The Antria star cluster is dominated by two giant elliptical galaxies: NGC 3268 (center) and NGC 3258 (bottom right). Image credits: Dark Energy Survey / DOE / FNAL / DECam / CTIO / NOIRLab / NSF / AURA / R. Colombari & M. Zamani, NSF's NOIRLab.

Galaxy clusters, like stars and galaxies, are fundamental building blocks of the universe.

These structures typically contain thousands of galaxies of all ages, shapes, and sizes.

They have a mass about a million times the mass of the Sun and are formed over billions of years as groups of small galaxies slowly come together.

At one point, galaxy clusters were believed to be the largest structures in the universe, until they were supplanted by the discovery of superclusters in the 1980s. Its length spans hundreds of millions of light years.

However, there is one thing the cluster holds on to. Because superclusters are not held together by gravity, galaxy clusters still hold the title of the largest gravitationally bound structures in the universe.

“Galaxy clusters are some of the largest known structures in the known universe,” NOIRLab astronomers said in a statement.

“Current models suggest that these giant structures form as clumps of dark matter, and that the galaxies that form within them are pulled together by gravity to form groups of dozens of galaxies, which then merge to form groups of several dozen galaxies. This suggests that they form clusters of hundreds or even thousands of galaxies.

“One such group is antoria clusterlocated approximately 130 million light-years from Earth in the direction of the constellation Antolia. ”

The Antlia cluster, also known as Abell S636, 3rd closest Add it to the local group after the Virgo and Fornax clusters.

The new images of the Antolia star cluster were captured by the Dark Energy Camera (DECam) mounted on NSF's Victor M. Blanco 4-meter telescope at Cerro Tololo Inter-American Observatory in Chile, a program of NSF's NOIRLab.

It captures only a portion of the 230 galaxies so far discovered to make up this cluster, as well as thousands of background galaxies.

“Antria Cluster” host Two giant elliptical galaxies: NGC3268 and NGC 3258,” the astronomers said.

“These central galaxies are surrounded by numerous faint dwarf galaxies.”

“Based on X-ray observations that revealed the existence of a 'rope' of globular clusters along the optical peak region between these two galaxies, we believe that these two galaxies are in the process of merging. Masu.”

“This may be evidence that the Antlia cluster is actually two smaller clusters joined together.”

“The cluster is rich in lenticular galaxies (a type of disk galaxy with little interstellar medium and therefore little continuous star formation), as well as some irregular galaxies,” the researchers added. .

“Many rarer, lower-luminosity dwarf galaxies have been discovered within this cluster, including ultracompact dwarfs, compact elliptical galaxies, and blue compact dwarfs.”

“The Antria cluster may also contain subtypes of dwarf spheroidal and superdiffuse galaxies, but further investigation is needed to confirm these.”

“Many of these galaxy types have been identified within the past few decades, as advances in observational instruments and data analysis techniques have allowed us to better capture the low luminosity and relatively small size of these galaxies. It just happened.”

“Assessing galaxy types allows us to plot details of their evolution, and some galaxies are rich in dark matter, providing further opportunities to understand this mysterious material, which makes up 25% of the universe. We will provide it.”

Source: www.sci.news