Spiralling Stars Provide a Window Into The Early Universe
Astronomers have been bemused to find young stars spiralling into the centre of a massive cluster of stars in the Small Magellanic Cloud, a satellite galaxy of the Milky Way. The outer arm of the spiral in this huge, oddly shaped stellar nursery — called NGC 346 — may be feeding star formation in a river-like motion of gas and stars. This is an efficient way to fuel star birth, researchers say.
The Small Magellanic Cloud has a simpler chemical composition than the Milky Way, making it similar to the galaxies found in the younger Universe, when heavier elements were more scarce. Because of this, the stars in the Small Magellanic Cloud burn hotter and so run out of their fuel faster than in our Milky Way. Though a proxy for the early universe, at 200 000 light-years away the Small Magellanic Cloud is also one of our closest galactic neighbours.
Learning how stars form in the Small Magellanic Cloud offers a new twist on how a firestorm of star birth may have occurred early in the history of the Universe, when it was undergoing a ‘baby boom’ about two to three billion years after the Big Bang (the Universe is now 13.8 billion years old).
The new results show that the process of star formation there is similar to that in our own Milky Way.
Only 150 light-years in diameter, NGC 346 boasts the mass of 50 000 Suns. Its intriguing shape and rapid star formation rate have puzzled astronomers. It took the combined power of the NASA/ESA Hubble Space Telescope and the European Southern Observatory’s Very Large Telescope (VLT) to unravel the behaviour of this mysterious-looking stellar nesting ground.
“Stars are the machines that sculpt the Universe. We would not have life without stars, and yet we don’t fully understand how they form,” explained study leader Elena Sabbi of the Space Telescope Science Institute in Baltimore. “We have several models that make predictions, and some of these predictions are contradictory. We want to determine what is regulating the process of star formation, because these are the laws that we need to also understand what we see in the early Universe.”
Researchers determined the motion of the stars in NGC 346 in two different ways. Using Hubble, Sabbi and her team measured the changes in the stars’ positions over 11 years. The stars in this region are moving at an average velocity of 3200 kilometres per hour, which means that in 11 years they move 320 billion kilometres. This is about twice the distance between Earth and the Sun.
But this cluster is relatively far away, inside a neighbouring galaxy. This means the observed motion is very small and therefore difficult to measure. These extraordinarily precise observations were possible only because of Hubble’s exquisite resolution and high sensitivity. Also, Hubble’s three-decade-long history of observations provides a baseline for astronomers to follow minute celestial motions over time.
The second team, led by Peter Zeidler of AURA/STScI for the European Space Agency, used the ground-based VLT’s Multi Unit Spectroscopic Explorer (MUSE) instrument to measure radial velocity, which determines whether an object is approaching or receding from an observer.
“What was really amazing is that we used two completely different methods with different facilities and basically we came to the same conclusion independently,” said Zeidler. “With Hubble, you can see the stars, but with MUSE we can also see the gas motion in the third dimension, and it confirms the theory that everything is spiralling inwards.”
But why a spiral?
“A spiral is really the good, natural way to feed star formation from the outside towards the centre of the cluster,” explained Zeidler. “It’s the most efficient way that stars and gas fuelling more star formation can move towards the centre.”
Half of the Hubble data for this study of NGC 346 is archival. The first observations were taken 11 years ago. They were recently repeated to trace the motion of the stars over time. Given the telescope’s longevity, the Hubble data archive now contains more than 32 years of astronomical data, powering unprecedented, long-term studies.
“The Hubble archive is really a gold mine,” said Sabbi. “There are so many interesting star-forming regions that Hubble has observed over the years. Given that Hubble is performing so well, we can actually repeat these observations. This can really advance our understanding of star formation.”
Observations with the NASA/ESA/CSA James Webb Space Telescope should be able to resolve lower-mass stars in the cluster, giving a more holistic view of the region. Over Webb’s lifespan, astronomers will be able to repeat this experiment and measure the motion of the low-mass stars. They will then be able to compare the high-mass stars and the low-mass stars to finally learn the full extent of the dynamics of this nursery.
More information
The Hubble Space Telescope is a project of international cooperation between ESA and NASA.
The teams’ findings appear on 8 September in the Astrophysical Journal.
The international team of astronomers in Sabbi’’s study consists of E. Sabbi (Space Telescope Science Institute, USA), P. Zeidler (AURA/STScI for the European Space Agency, Space Telescope Science Institute, USA), R.P. van der Marel (Space Telescope Science Institute, USA), A. Nota (Space Telescope Science Institute, USA), J. Anderson (Space Telescope Science Institute, USA), J.S. Gallagher (Department of Astronomy, University of Wisconsin–Madison, USA), D.J. Lennon (Instituto de Astrofísica de Canarias, Spain; Department of Astrophysics, University of La Laguna, Spain), L.J. Smith (Space Telescope Science Institute, USA), and M. Gennaro (Space Telescope Science Institute, USA).
The international team of astronomers in Zeidler’s study consists of P. Zeidler (AURA/STScI for the European Space Agency, Space Telescope Science Institute, USA), E. Sabbi (Space Telescope Science Institute, USA), and A. Nota (Space Telescope Science Institute, USA).
Image Credit: NASA, ESA
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