The recipe for star clusters: Take one gas cloud 500 light years in diameter, add 5 million years, process for one month

June 25, 2018, McMaster University
A snapshot of a simulated giant molecular cloud marked with with star clusters in formation. Credit: McMaster University

Clusters of stars across the vast reaches of time and space of the entire universe were all created the same way, researchers at McMaster University have determined.

Researchers Corey Howard, Ralph Pudritz and William Harris, authors of a paper published June 25 in the journal Nature Astronomy, used highly-sophisticated computer simulations to re-create what happens inside gigantic clouds of concentrated gases known to give rise to clusters of that are bound together by gravity.

Pudritz and Harris, both professors of Physics and Astronomy at McMaster, were Howard's Ph.D. thesis supervisors and guided his research. Howard recently completed post-doctoral research at the university.

The state-of-the-art simulations follow a cloud of interstellar gas 500 light years in diameter, projecting 5 million years' worth of evolution wrought by turbulence, gravity and feedback from intense radiation pressure produced by massive stars within forming clusters.

The research shows how those forces create dense filaments that funnel gas into what ultimately become super-bright clusters of stars that can merge with other clusters to form vast globular clusters.

"Most stars in galaxies form as members of star clusters within dense molecular clouds, so one of the most basic questions in astronomy is how do clusters that range from hundreds to millions of stars form under a wide variety of conditions," Pudritz says. "Our simulations were carefully designed to determine whether or not this a universal process."

The authors programmed data for such variables as gas pressure, space turbulence and radiation force into their and let it run using resources that included SciNet, Canada's largest supercomputer centre.

After a month, the program turned out star clusters identical to those known to exist, showing that the researchers had managed to reverse-engineer the formation of star clusters, taking a major step towards understanding their formation, which has long been a subject of debate among astrophysicists.

"Our work shows that, given a large enough collection of gas, a massive star is the natural outcome," Howard says. "Since massive star clusters trace the conditions of the galaxies in which they form, we may also be able use this knowledge to reverse-engineer the conditions in the distant universe."

Many had previously argued that clusters of different sizes and ages had formed differently, the authors said, but the new research shows they all form the same way.

The simulations show that the outcome depends on the initial reservoir of gas, that will, after turbulence, gravity and feedback have done their work, create clusters of stars of various sizes over the course of a few million years.

"This is the first convincing route to modelling the formation of ," Harris says. "It applies across all mass scales—little clusters and big ones—and it should work at any particular time in the universe's history, in any particular galaxy."

Such simulations would have been unthinkable even 10 years ago, the authors say. The success of this project, they say, suggests that similar research on other complex problems, such as the formation of entire galaxies down to the births of specific individual stars, could soon be within reach.

Explore further: Old star clusters could have been the birthplace of supermassive stars

More information: Corey S. Howard et al, A universal route for the formation of massive star clusters in giant molecular clouds, Nature Astronomy (2018). DOI: 10.1038/s41550-018-0506-0

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Francis Bacon
1 / 5 (1) Jun 27, 2018
Questions:
Even with all that computer power, wouldn't some shortcuts be necessary to simulate all that? A lot of averaging, assuming certain things, etc.?

If it was based on "turbulence, gravity and feedback from intense radiation pressure produced by massive stars within forming clusters," how did those massive stars form?

Did they take into account Dark Matter? And on a scale of 500 light years, wouldn't Dark Energy have an effect?
Ojorf
1 / 5 (3) Jun 28, 2018
Yes, the simulation will never have the resolution of the real thing. It's not so much a question of short-cuts, but a trade-off between how detailed the simulation is vs how long it takes to run.

I'm no quite sure, but I think they might have run a bunch of simulations with varying input parameters (say various initial clump masses and accretion rates) to determine the closest fit to real observations.

DE would have no affect at these scales and I assume DM might affect initial clump masses and accretion rates, so would automatically be included by picking the simulation that accords with reality.

Nothing is mentioned in the abstract concerning any details of the simulations, hopefully someone with more insight (and access to the article) can let us know.

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