A thread of the cosmic web: Astronomers spot a 50 million light-year galactic filament
At the very largest scale, the Universe consists of a "cosmic web" made of enormous, tenuous filaments of gas stretching between gigantic clumps of matter. Or that's what our best models suggest. All we have seen so far with our telescopes are the stars and galaxies in the clumps of matter.
So is the cosmic web real, or a figment of our models? Can we confirm our models by detecting these faint gaseous filaments directly?
Until recently, these filaments have been elusive. But now a collaboration between Australian radio astronomers and German X-ray astronomers has detected one.
CSIRO's newly completed Australian Square Kilometre Array Pathfinder (ASKAP) telescope in Western Australia is starting to produce a large-scale picture of the Universe in radio frequencies. This telescope can see deeper than any other radio telescope, producing new discoveries, such as the unexplained Odd Radio Circles or ORCs.
Seeing with radio waves and X-rays
This year has also seen the publication of the first observations by the German eROSITA Space Telescope, which is giving us our deepest large-scale picture of the Universe in X-ray frequencies. Both of these next-generation telescopes have an unprecedented ability to scan large areas of sky at once, so they are beautifully matched to study the large-scale features of the Universe. Together, they can achieve much more than either on its own, so naturally we have joined forces.
The first result from this collaboration is the discovery of a cosmic filament of hot gas. This study was led by Thomas Reiprich of the University of Bonn and Marcus Brueggen of the University of Hamburg, and involved Australian scientists from CSIRO and from Curtin, Macquarie, Monash and Western Sydney universities. It is published today in two papers in the journal Astronomy and Astrophysics.
The cosmic web
The Big Bang 13.8 billion years ago produced a Universe filled with invisible dark matter, together with a featureless gas of hydrogen and helium, and little else. Over the next few billion years, the gas clumped together under the attraction of gravity, forming filaments of matter with vast empty voids between them. The filaments probably contain more than half the matter in the Universe, even though the filaments themselves contain just ten particles per cubic meter—less than the best vacuum we can create on Earth.
Nearly all the galaxies we see today, including our own Milky Way, are thought to have formed in these filaments. We think galaxies then slide along the filaments until they fall into the dense clusters of galaxies clumped together at junctions where filaments meet.
But until now, all this was hypothetical—we could see the galaxies and clusters, but we couldn't see the gaseous filaments themselves. Now, eROSITA has directly detected the hot gas in a filament 50 million light-years long. This is an important step forward, confirming our model of the cosmic web is correct.
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eROSITA image showing the clusters at the centre, and the dark green gaseous filament stretching 50 million light-years from the bottom left to the top right. Credit: Thomas Reiprich -
This image, from a simulation called Magneticum, shows clumps moving along filaments, merging with the main systems to form ever larger, denser, and hotter structures. Credit: Thomas Reiprich -
Large-scale evolution of the A3391/95 analog found in the Magneticum simulation. The gas density distribution is shown in a cubic cutout region of 20 Mpc/h per side around the redshift of the main system in comoving coordinates from redshift z~1 to z~0.07. We note the clumps falling in along the large-scale filaments, merging with the main systems to form ever larger, denser, and hotter structures. Credit: Reiprich et al., Astronomy & Astrophysics
A smooth ride
We also expected the hot gas would whip up electrons to produce radio frequency emissions, but, curiously, we don't detect the filament with ASKAP. This tells us the hot gas is flowing smoothly, without the turbulence that would accelerate electrons to produce radio waves. So the galaxies are getting a smooth ride as they fall into the clusters.
We can see the individual galaxies falling into the clusters in the radio images from ASKAP. At radio wavelengths, we often see galaxies bracketed by a pair of jets, caused by electrons squirting out from near the black hole in the center of the galaxy.
However, in our radio images of these clusters, we see the jets bent and distorted as they are buffeted by intergalactic winds in the dense gas in the clusters. Again, this is a good confirmation of our models.
This work is not only important as confirmation of our model of the Universe, but is also the first result to come from the collaboration between ASKAP and eROSITA. These two telescopes are beautifully matched to survey our Universe, seeing the Universe as it has never been seen before, and I expect this discovery to be the first of many.
More information: Radio observations of the merging galaxy cluster system Abell 3391-Abell 3395, arXiv:2012.08775 [astro-ph.HE] arxiv.org/abs/2012.08775
The Abell 3391/95 galaxy cluster system: A 15 Mpc intergalactic medium emission filament, a warm gas bridge, infalling matter clumps, and (re-) accelerated plasma discovered by combining SRG/eROSITA data with ASKAP/EMU and DECam data, arXiv:2012.08491 [astro-ph.CO] arxiv.org/abs/2012.08491
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