This article has been reviewed according to Science X's editorial process and policies. Editors have highlighted the following attributes while ensuring the content's credibility:


peer-reviewed publication


Giant galactic explosion exposes galaxy pollution in action

Giant galactic explosion exposes galaxy pollution in action
Galaxy NGC 4383 evolving strangely. Gas is flowing from its core at a rate of over 200 km/s. This mysterious gas eruption has a unique cause: star formation. Credit: ESO/A. Watts et al

A team of international researchers studied galaxy NGC 4383, in the nearby Virgo cluster, revealing a gas outflow so large that it would take 20,000 years for light to travel from one side to the other.

The discovery is published in the journal Monthly Notices of the Royal Astronomical Society.

Lead author Dr. Adam Watts, from The University of Western Australia node at the International Centre for Radio Astronomy Research (ICRAR), said the was the result of powerful stellar explosions in the central regions of the galaxy that could eject enormous amounts of hydrogen and heavier elements.

The mass of gas ejected is equivalent to more than 50 million suns.

Researchers Dr. Adam Watts and Professor Barbara Catinella discuss the discovery and gas pollution in space. Credit: ICRAR

"Very little is known about the physics of outflows and their properties because outflows are very hard to detect," Dr. Watts said.

"The ejected gas is quite rich in giving us a unique view of the complex process of mixing between hydrogen and metals in the outflowing gas.

"In this particular case, we detected oxygen, nitrogen, sulfur and many other chemical elements."

Gas outflows are crucial to regulate how fast and for how long can keep forming stars. The gas ejected by these explosions pollutes the space between stars within a galaxy, and even between galaxies, and can float in the intergalactic medium forever.

The high-resolution map was produced with data from the MAUVE survey, co-led by ICRAR researchers Professors Barbara Catinella and Luca Cortese, who were also co-authors of the study.

The survey used the MUSE Integral Field Spectrograph on the European Southern Observatoryʼs Very Large Telescope, located in northern Chile.

"We designed MAUVE to investigate how such as gas outflows help stop in galaxies," Professor Catinella said.

"NGC 4383 was our first target, as we suspected something very interesting was happening, but the data exceeded all our expectations.

"We hope that in the future, MAUVE observations reveal the importance of gas outflows in the local universe with exquisite detail."

More information: Adam Watts et al, MAUVE: A 6 kpc bipolar outflow launched from NGC 4383, one of the most HI-rich galaxies in the Virgo cluster, Monthly Notices of the Royal Astronomical Society (2024). DOI: 10.1093/mnras/stae898

Provided by International Centre for Radio Astronomy Research

Citation: Giant galactic explosion exposes galaxy pollution in action (2024, April 21) retrieved 25 May 2024 from
This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no part may be reproduced without the written permission. The content is provided for information purposes only.

Explore further

Astronomers discover 49 new galaxies in under three hours


Feedback to editors