Blog icon

29 June 2021 Partner Release

An international group of astronomers has created images with never-before-seen detail of a galaxy cluster with a black hole at its centre, travelling at high speed along an intergalactic ‘road of matter’. The findings also support existing theories of the origins and evolution of the universe.

The concept that roads of thin gas connect clusters of galaxies across the universe has been difficult to prove until recently, because the matter in these ‘roads’ is so sparse it eluded the gaze of even the most sensitive instruments. Following the 2020 discovery of an intergalactic thread of gas at least 50 million light-years long, scientists have now developed images with an unprecedented level of detail of the ‘Northern Clump’ – a cluster of galaxies found on this thread.

By combining imagery from various sources including CSIRO’s ASKAP radio telescope, SRG/eROSITA, XMM-Newton and Chandra satellites, and DECam optical data, the scientists could make out a large galaxy at the centre of the clump, with a black hole at its centre.

In a press conference overnight, the eROSITA team at the University of Bonn presented their observations of the clump, which appears to be moving at high speed. Jets of matter are streaming out behind it “like the braids of a running girl,” says lead author of the study, Angie Veronica from the Argelander Institute for Astronomy at the University of Bonn.

The leader of the EMU project, which contributed data from ASKAP for the study, Professor Andrew Hopkins of Australian Astronomical Optics, Macquarie University, says, “The excellent sensitivity of the ASKAP telescope to faint extended radio emission is the key that allows the detection of these jets of radio emission from the supermassive black hole. The shape and orientation of these jets in turn provide important clues to the motion of the galaxy hosting the black hole.”

Professor Thomas Reiprich of the University of Bonn says, “We are currently interpreting this observation such that the Northern Clump is losing matter as it travels. However, it could also be that even smaller clumps of matter in the thread are falling toward the Northern Clump.”

Overall, the observations confirm the theoretical view that the gas filament is an intergalactic road of matter. The Northern Clump is moving along this road at high speed toward two other, much larger galaxy clusters called Abell 3391 and Abell 3395.

“It's sort of falling into these clusters and will continue to enlarge them — just like the principle of ‘winner takes all’,” says Professor Reiprich. “What we're seeing is a snapshot of that fall.”

This story originally appeared on the Macquarie University news site: Images emerge of galaxies headed for collision


Swept back gas from this large galaxy in the Abell galaxy cluster system indicate that it is moving ©  Veronica et al.

Contact us

Find out how we can help you and your business. Get in touch using the form below and our experts will get in contact soon!

CSIRO will handle your personal information in accordance with the Privacy Act 1988 (Cth) and our Privacy Policy.

First name must be filled in

Surname must be filled in

I am representing *

Please choose an option

Please provide a subject for the enquriy

0 / 100

We'll need to know what you want to contact us about so we can give you an answer

0 / 1900

You shouldn't be able to see this field. Please try again and leave the field blank.