GIANT GALAXIES that contain billions of stars are born in much the same way as delicate snowflakes, new research from Swinburne University of Technology has shown.
In a paper accepted for publication in the Monthly Notices of the Royal Astronomical Society, Professor Duncan Forbes has provided the first direct evidence to support a theory of galaxy formation that he has likened to the birth of a snowflake.
Forbes, with the help of international collaborators, analysed data from three different telescopes in order to help confirm this galaxy formation theory proposed last year by German astronomer Ludwig Oser and his colleagues.
“What we’ve found is that galaxies form in two phases. Firstly, an inner region of stars is formed from collapsing gas. This region then acts as a core, or ‘seed’, around which the galaxy grows as the result of stars which are acquired from other smaller galaxies,” he said.
According to Professor Jean Brodie from the University of California, “our work provides some of the best evidence for this inside-out build up of giant galaxies.”
What intrigued the astronomers was the similarity between this inside-out process for giant galaxy formation and the way that snowflakes are formed.
“Snowflake formation requires a ‘seed’ to get it started. In the case of snowflakes, that ‘seed’ is a microscopic dust grain. Having a core from which to build upon is comparable to the formation of a giant galaxy,” Forbes said.
Big telescopes study big galaxies
The astronomers based their conclusions on observations of the massive elliptical galaxy NGC1407, one of the largest galaxies in the southern skies with over 10 billion stars.
They made their observations using two giant telescopes in Hawaii—the 8.2-metre Subaru and the 10-metre Keck, the largest optical telescope in the world. They also included data collected from the Hubble Space Telescope.
“Our data came from three of the world’s premier telescopes, and in each case it supported the ‘snowflake theory’ of galaxy formation,” Forbes said. “This means we can be very confident in our findings.”
Observations at the Keck telescope are made possible thanks to Swinburne’s agreement with the California Institute of Technology (Caltech) that gives Swinburne astronomers access to the telescopes for up to 20 nights per year.
The research paper was led by Professor Duncan Forbes, and co-authored by Dr Lee Spitler and Caroline Foster from Swinburne University, Dr Jay Strader from the Harvard-Smithsonian Centre for Astrophysics and Professor Jean Brodie and Dr Aaron Romanowsky from the University of California at Santa Cruz.
Adapted from information issued by Swinburne University. Image credit: Keck Observatory and Subaru Observatory.
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