The complex mechanics determining how galaxies spin, grow, cluster and die have been revealed following the release of all the data gathered during a massive seven-year Australian-led astronomy research project.
The scientists observed 13 galaxies at a time, building to a total of 3068, using a custom-built instrument called the Sydney-AAO Multi-Object Integral-Field Spectrograph (SAMI), connected to the 4-metre Anglo-Australian Telescope (AAT) at Siding Spring Observatory in New South Wales. The telescope is operated by the Australian National University.
Overseen by the ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), the project used bundles of optical fibres to capture and analyse bands of colours, or spectra, at multiple points in each galaxy.
The results allowed astronomers from around the world to explore how these galaxies interacted with each other, and how they grew, sped up or slowed down over time.
No two galaxies are alike. They have different bulges, haloes, disks and rings. Some are forming new generations of stars, while others haven’t done so for billions of years. And there are powerful feedback loops in them fuelled by supermassive black holes.
Professor Scott Croom from ASTRO 3D and the University of Sydney explained:
“The SAMI survey lets us see the actual internal structures of galaxies, and the results have been surprising.
“The sheer size of the SAMI Survey lets us identify similarities as well as differences, so we can move closer to understanding the forces that affect the fortunes of galaxies over their very long lives.”
The survey, which began in 2013, has already formed the basis of dozens of astronomy papers, with several more in preparation. A paper describing the final data release – including, for the first time, details of 888 galaxies within galaxy clusters – was published on the arxiv pre-print server and in the journal Monthly Notices of the Royal Astronomical Society.
“The nature of galaxies depends both on how massive they are and their environment,” said Professor Croom.
“For example, they can be lonely in voids, or crowded into the dense heart of galactic clusters, or anywhere in between. The SAMI Survey shows how the internal structure of galaxies is related to their mass and environment at the same time, so we can understand how these things influence each other.”
Research arising from the survey has already revealed several unexpected outcomes.
One group of astronomers showed that the direction of a galaxy’s spin depends on the other galaxies around it, and changes depending on the galaxy’s size. Another group showed that the amount of rotation a galaxy has is primarily determined by its mass, with little influence from the surrounding environment. A third looked at galaxies that were winding down star-making, and found that for many the process began only a billion years after they drifted into the dense inner-city regions of clusters.
Dr Matt Owers from Macquarie University in Australia explained:
“The SAMI Survey was set up to help us answer some really broad top-level questions about galaxy evolution.
“The detailed information we’ve gathered will help us to understand fundamental questions such as: Why do galaxies look different depending on where they live in the Universe? What processes stop galaxies forming new stars and, conversely, what processes drive the formation of new stars? Why do the stars in some galaxies move in a highly ordered rotating disk, while in other galaxies their orbits are randomly oriented?”
Professor Croom added:
“The survey is finished now, but by making it all public we hope that the data will continue to bear fruit from many, many years to come.”
Co-author Associate Professor Julia Bryant from ASTRO 3D and the University of Sydney said:
“The next steps in this research will make use of a new Australian instrument – which we’ve called Hector – that will start operation in 2021, increasing the detail and number of galaxies that can be observed.”
When fully installed in the AAT, Hector will survey 15,000 galaxies.