ASTRONOMERS at ANU have created the most detailed radio image of nearby dwarf galaxy, the Small Magellanic Cloud, revealing secrets of how it formed and how it’s likely to evolve. 

The image was taken by CSIRO’s new radio telescope, the Australian Square Kilometre Array Pathfinder (ASKAP), and its innovative radio camera technology, known as “phased array feeds”.

The Small Magellanic Cloud, which is a tiny fraction of the size and mass of the Milky Way, is one of our nearest galactic neighbours and visible to the naked eye in the southern sky.

Co-lead researcher Prof Naomi McClure-Griffiths says the complex structure of the dwarf galaxy likely resulted, in part, from interactions with its companion, the Large Magellanic Cloud, and the Milky Way.

“The new image captured by CSIRO’s Australian Square Kilometre Array Pathfinder telescope reveals more gas around the edges of the galaxy, indicating a very dynamic past for the Small Magellanic Cloud,” she says.

“These features are more than three times smaller than we were able to see before and allow us to probe the detailed interaction of the small galaxy and its environment.”

The new image was created as part of a survey that aims to study the evolution of galaxies.

Prof McClure-Griffiths says distortions to the Small Magellanic Cloud occurred because of its interactions with the larger galaxies and because of its own star explosions that push gas out of the galaxy.

“The outlook for this dwarf galaxy is not good, as it’s likely to eventually be gobbled up by our Milky Way,” she says.

“Together, the Magellanic Clouds are characterised by their distorted structures, a bridge of material that connects them, and an enormous stream of hydrogen gas that trails behind their orbit – a bit like a comet.”

The Small Magellanic Cloud has been studied extensively in the past few years by infrared telescopes such as NASA’s Spitzer Space Telescope and ESA’s Herschel telescope, which study the dust and stars within the galaxy.

“The new radio image finally reaches the same level of detail as those infrared images, but on a very different component of the galaxy’s make-up: its hydrogen gas,” Prof McClure-Griffiths says.

“Hydrogen is the fundamental building block of all galaxies and shows off the more extended structure of a galaxy than its stars and dust.”

CSIRO’s Dr Philip Edwards, says the stunning image showcases the wide field of view of the ASKAP telescope, and augurs well for when the full array will come on-line next year.”