Galaxies with extended disks maintain productivity, research reveals
Massive galaxies with extra-large extended “puffy” disks produced stars for longer than their more compact cousins, new modelling reveals.
In a paper published in the Astrophysical Journal, researchers led by Dr Anshu Gupta and Associate Professor Kim-Vy Tran from Australia’s ARC Centre of Excellence in All Sky Astrophysics in 3 Dimensions (ASTRO 3D), show that the sheer size of a galaxy influences when it stops making new stars.
“There’s a period in the life of the Universe known as the ‘cosmic noon’, which occurred about 10 billion years ago,” said Dr Gupta.
“That was when star formation in massive galaxies was at its peak. After that, gas in most of these galaxies grew hot – in part because of the black holes in the middle of them – and they stopped forming stars.
“In galaxies that are really, really stretched out, however, we found that things didn’t heat up as much and the black holes didn’t exert such a great influence, so stars kept getting made over a longer period.”
Dr Gupta and Dr Tran, both of whom are based at the University of NSW, Sydney, found that they could predict the end of star formation based on the size of a galaxy’s disk – the flat, circular region surrounding its centre, comprising stars, hydrogen gas and dust.
“Where the stars in the disk are widely distributed – you could call it ‘puffy’ – the gas stays cooler, so continues to coalesce under gravity and form new stars,” said Dr Gupta.
“In galaxies with more compact disks, the gas heats up quite quickly and is soon too energetic to mash together, so the formation of stars finishes by just after cosmic noon. Puffy disks keep going much longer, say as far as cosmic afternoon tea.”
To make their findings, the researchers, with colleagues from Melbourne, Germany, Mexico and the United States, used cosmological galaxy formation simulations from an international collaboration known as the IllustrisTNG project.
This was integrated with deep observations from an Australian-led project known as the Multi-Object Spectroscopic Emission Line (MOSEL) Survey.
“The IllustrisTNG simulations required millions of hours of supercomputer time,” said Dr Tran.
“And the MOSEL survey needs both the WM Keck Observatory in Hawai’i and the Hubble Space Telescope.
“The results mean that for the first time we’ve been able to establish a relationship between disk size and star-making. So now astronomers will be able to look at any galaxy in the Universe and accurately predict when it will stop making stars – just after lunch, or later in the cosmic afternoon.”
The Milky Way, incidentally, is a massive galaxy that is still making stars. That’s because it was something of a cosmic late-starter. When cosmic noon arrived it was very small – containing only one-tenth of the star mass it hosts today – and did not attain ‘massive’ status until much, much later.
As a result, the gas and dust within it has not yet warmed up enough to quench the star-making process.
It is not, however, an extended puffy galaxy, so it will quench, relatively speaking, sooner rather than later.
“Cosmic noon was a long time ago,” said Dr Gupta. “I’d say that by now the Universe has reached cosmic evening. It’s not night-time yet, but things have definitely slowed down.”
As well as UNSW, team members hailed from Swinburne University, the Max-Planck-Institut fur Astronomie, the Universidad Nacional Autonoma de Mexico, and the Flatiron Institute and Columbia University, both in New York.
An ensemble of twenty-five disk galaxies. The view on the left shows light emitted in the H-alpha line from interstellar gas as a result of ongoing star-formation, while the panels on the right shows the optical light emitted by a mix of young (bluer) and old (redder) stars. Each galaxy can be seen rotated edge-on below its face-on view.
Credit: TNG Collaboration
A graph showing how extended or ‘puffy’ galaxies continue to make stars longer into the cosmic afternoon than compact ones.
Credit: Anshu Gupta
MOSEL and IllustrisTNG: Massive Extended Galaxies at z = 2 Quench Later Than Normal-size Galaxies
Arxiv version, full paper: https://arxiv.org/abs/2011.08198
Authors: Anshu Gupta (1, 2), Kim-Vy Tran (1, 2), Annalisa Pillepich (3), Tiantian Yuan (4, 2), Anishya Harshan (1, 2), Vicente Rodriguez-Gomez (5), and Shy Genel (6, 7)
1 School of Physics, University of New South Wales, Sydney, Australia
2 ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Australia
3 Max-Planck-Institut fur Astronomie, Heidelberg, Germany
4 Swinburne University of Technology, Hawthorn, Australia
5 Instituto de Radioastronomıa y Astrofısica, Universidad Nacional Autonoma de Mexico, Mexico
6 Center for Computational Astrophysics, Flatiron Institute, New York, USA
7 Columbia Astrophysics Laboratory, Columbia University, New York, USA
More about ASTRO 3D:
ASTRO 3D is a seven-year $40 million Centre of Excellence project funded by the Australian Government through the Australian Research Council. The Centre began in June 2017 and will end in June 2024. It hosts around 200 investigators and professional staff, mostly based at six nodes: the Australian National University, Curtin University, Swinburne University of Technology, University of Melbourne, University of Sydney, and University of Western Australia. https://astro3d.org.au/
More about the MOSEL survey: https://sites.google.com/view/moselsurvey/home