Showing posts with label Giant Radio Galaxies (GRGs). Show all posts
Showing posts with label Giant Radio Galaxies (GRGs). Show all posts

Friday, January 31, 2025

'Troublesome' radio galaxy 32 times size of Milky Way spotted

The newly-discovered giant radio galaxy ‘Inkathazo’. The glowing plasma jets, as seen by the MeerKAT telescope, are shown in red and yellow. The starlight from other surrounding galaxies can be seen in the background. Credit: K.K.L Charlton (UCT), MeerKAT, HSC, CARTA, IDIA
Licence type: Attribution (CC BY 4.0)

Astronomers have discovered an extraordinary new giant radio galaxy with plasma jets 32 times the size of our Milky Way.

Measuring 3.3 million light-years from end-to-end, the cosmic megastructure was spotted by South Africa's MeerKAT telescope and nicknamed Inkathazo – meaning 'trouble' in the African Xhosa and Zulu languages – because of the difficulty in understanding the physics behind it.

Researchers hope their "exciting and unexpected discovery", published today in Monthly Notices of the Royal Astronomical Society, will shed light on the mysterious origin and evolution of what are some of the largest structures in the Universe.

Giant radio galaxies (GRGs) are cosmic behemoths spewing jets of hot plasma millions of light-years across intergalactic space. These plasma jets, which glow at radio frequencies, are powered by supermassive black holes at the centres of galaxies.

Until recently, GRGs were thought to be quite rare. However, a new generation of radio telescopes, such as South Africa's MeerKAT, have since turned this idea on its head.

"The number of GRG discoveries has absolutely exploded in the past five years thanks to powerful new telescopes like MeerKAT," said Kathleen Charlton, a Master’s student at the University of Cape Town and the first author of the new study.

"Research into GRGs is developing so rapidly that it's becoming hard to keep up. It's incredibly exciting!"

A spectral age map of ‘Inkathazo’. Cyan and green show younger plasma, while purple indicates older plasma. K.K.L Charlton (UCT), MeerKAT, HSC, CARTA, IDIA
Licence type: Atribution (CC BY 4.0)

She added: "We nicknamed this giant galaxy 'Inkathazo,' meaning 'trouble' in isiZulu and isiXhosa because it has been a bit troublesome to understand the physics behind what’s going on here.

"It doesn't have the same characteristics as many other giant radio galaxies. For example, the plasma jets have an unusual shape: rather than extending straight across from end-to-end, one of the jets is bent."

Inkathazo also lives at the very heart of a cluster of galaxies, rather than in relative isolation, which should make it difficult for the plasma jets to grow to such enormous sizes.

"This is an exciting and unexpected discovery," said Dr Kshitij Thorat, a co-author of the study from the University of Pretoria.

"Finding a GRG in a cluster environment raises questions about the role of environmental interactions in the formation and evolution of these giant galaxies."

To try and understand more about this cosmic conundrum, the researchers took advantage of MeerKAT’s exceptional capabilities to create some of the highest-resolution spectral age maps ever made for GRGs. These maps track the age of the plasma across different parts of the GRG, providing clues about the physical processes at work.

The results revealed intriguing complexities in Inkathazo’s jets, with some electrons receiving unexpected boosts of energy. The researchers believe this may occur when the jets collide with hot gas in the voids between galaxies in a cluster.

"This discovery has given us a unique opportunity to study GRG physics in extraordinary detail," said Thorat. "The findings challenge existing models and suggest that we don’t yet understand much of the complicated plasma physics at play in these extreme galaxies."

South Africa's MeerKAT telescope.
South African Radio Astronomy Observatory
Licence type: Attribution (CC BY 4.0)

Most known GRGs have been found at northern latitudes with European telescopes, while the southern sky remains relatively unexplored for such giant objects. Yet Inkathazo is not alone. It is the third GRG to be spotted in a small patch of sky, around the size of five full moons, that astronomers refer to as 'COSMOS'.

When an international team of astronomers named the 'MIGHTEE' collaboration observed COSMOS with the MeerKAT telescope, they immediately spotted the other two other GRGs and published their findings in 2021.

Inkathazo was seen more recently in follow-up observations with MeerKAT, which is operated by the South African Radio Astronomy Observatory.

"The fact that we unveiled three GRGs by pointing MeerKAT at a single patch of sky goes to show that there is likely a huge treasure trove of undiscovered GRGs in the southern sky" said Dr Jacinta Delhaize, a researcher at the University of Cape Town, who led the 2021 publication.

"MeerKAT is incredibly powerful and in a perfect location, so is excellently poised to uncover and learn more about them."

As a precursor to the Square Kilometre Array (SKA) due to begin operations at the end of this decade, MeerKAT offers unprecedented sensitivity and resolution, enabling discoveries like Inkathazo.

"We're entering an exciting era of radio astronomy," said Dr Delhaize. "While MeerKAT has taken us further than ever before, the SKA will allow us to push these boundaries even further and hopefully solve some of the mysteries surrounding enigmatic objects like giant radio galaxies."

Submitted by Sam Tonkin




Media contacts

Sam Tonkin
Royal Astronomical Society
Mob: +44 (0)7802 877 700

press@ras.ac.uk

Dr Robert Massey
Royal Astronomical Society
Mob: +44 (0)7802 877 699

press@ras.ac.uk



Scientific contacts

Kathleen Charlton
University of Cape Town
Tel: +27 (0)832 603 855

CHRKAT009@myuct.ac.za

Dr Jacinta Delhaize
University of Cape Town

drjdelhaize@gmail.com

A/Prof Kshitij Thorat
University of Pretoria

kshitijthorat.astro@gmail.com



Further information

The paper ‘A spatially-resolved spectral analysis of giant radio galaxies with MeerKAT’ by Kathleen Charlton et al. has been published in Monthly Notices of the Royal Astronomical Society. DOI: 10.1093/mnras/stae2543

Notes for editors

About the MIGHTEE collaboration

This work was co-authored by several members of the international MIGHTEE collaboration of astronomers, led by Professor Matt Jarvis (University of Oxford) and with key contributions by Dr Ian Heywood (University of Oxford).

The MeerKAT International Gigahertz Tiered Extragalactic Exploration (MIGHTEE) survey is a Large Survey Project being conducted with the MeerKAT telescope. Its overarching goal is to study the formation and evolution of galaxies. For more information, visit
https://www.mighteesurvey.org/

About MeerKAT

The MeerKAT telescope is located in the Karoo region of South Africa and is comprised of 64 radio dishes. It is managed by the South African Radio Astronomy Observatory (SARAO), which is a facility of the National Research Foundation. Further details are available at: https://www.sarao.ac.za/science/meerkat/

About the Royal Astronomical Society

The Royal Astronomical Society (RAS), founded in 1820, encourages and promotes the study of astronomy, solar-system science, geophysics and closely related branches of science.

The RAS organises scientific meetings, publishes international research and review journals, recognises outstanding achievements by the award of medals and prizes, maintains an extensive library, supports education through grants and outreach activities and represents UK astronomy nationally and internationally. Its more than 4,000 members (Fellows), a third based overseas, include scientific researchers in universities, observatories and laboratories as well as historians of astronomy and others.

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Tuesday, March 19, 2013

LOFAR discovers new giant galaxy in all-sky survey


A team of astronomers led by ASTRON astronomer Dr. George Heald has discovered a previously unknown gigantic radio galaxy, using initial images from a new, ongoing all-sky radio survey. The galaxy was found using the powerful International LOFAR Telescope (ILT), built and designed by ASTRON. The team is currently performing LOFAR's first all-sky imaging survey, the Multi-frequency Snapshot Sky Survey (MSSS). While browsing the first set of MSSS images, Dr. Heald identified a new source the size of the full moon projected on the sky. The radio emission is associated with material ejected from one member of an interacting galaxy triplet system tens to hundreds of millions of years ago. The physical extent of the material is much larger than the galaxy system itself, extending millions of light years across intergalactic space. The MSSS survey is still ongoing, and is poised to discover many new sources like this one. 

The new galaxy is a member of a class of objects called Giant Radio Galaxies (GRGs). GRGs are a type of radio galaxy with extremely large physical size, suggesting that they are either very powerful or very old. LOFAR is an effective tool to find new GRGs like this one because of its extreme sensitivity to such large objects, combined with its operation at low frequencies that are well suited to observing old sources. 

The center of the new GRG is associated with one member of a galaxy triplet known as UGC 09555. The central galaxy is located at a redshift of z=0.054536, or 750 million light years from Earth. The central radio source was previously known and has a flat radio spectrum, typical of giant radio galaxies. 

LOFAR's MSSS survey is a concerted effort to image the entire northern sky at very low radio frequencies, between 30 and 160 MHz (wavelengths from 2m to 10m). The primary aim of the survey is to perform an initial shallow scan of the sky, in order to create an all-sky model that will support the calibration of much deeper observations. It is comparable in sensitivity and angular resolution to previous surveys with ‘classical' radio telescopes like the Very Large Array (VLA) in the USA, ASTRON's Westerbork Synthesis Radio Telescope (WSRT), and the Giant Metrewave Radio Telescope (GMRT) in India. MSSS is unique in that it operates at substantially lower frequencies, and is therefore poised to uncover new sources that were missed by previous surveys. Its broad bandwidth coverage is also novel in all-sky radio surveys, and will be used to provide additional information about the detected objects. 

The international team of astronomers that is performing the MSSS survey is made up of about fifty members from various institutes, mostly in the Netherlands, Germany, the UK, Poland, France and Italy.
 

 
For more information please contact:
 
Femke Boekhorst, PR & Communication. 
E-mail: boekhorst@astron.nl 
Phone: +31 521 595 204
Dr. George Heald, astronomer. 
E-mail: heald@astron.nl 
Phone: +31 521 595 100

Caption to the image: Overlay of the new GRG (blue-white colors) on an optical image from the Digitized Sky survey. The inset shows the central galaxy triplet (image from Sloan Digital Sky Survey). The image is about 2 Mpc across. 

More information about MSSS can be found on the ASTRON website: http://www.astron.nl/radio-observatory/lofar-msss/lofar-msss.