Magnetic waves create chaos in star-forming clouds

New research by Stella Offner, assistant professor of astronomy at The University of Texas at Austin, finds that magnetic waves are an important factor driving the process of star formation within the enormous clouds that birth stars.

Her research sheds light on the processes that are responsible for setting the properties of stars, which in turn affects the formation of planets orbiting them, and, ultimately, life on those planets. The research is published in the current issue of the journal Nature Astronomy.

Offner used a supercomputer to make models of the multitude of processes happening inside a cloud where stars are forming, in an effort to sort out which processes lead to which effects.

"These clouds are violent places," Offner said.

"It's an extreme environment with all kinds of different physics happening at once," including gravity and turbulence as well as radiation and winds from forming stars (called stellar feedback). The fundamental question, Offner said, is: "Why are the motions in these clouds so violent?"

Some astronomers attribute the observed motions to gravitational collapse, while others attribute it to turbulence and stellar feedback. Offner wanted to test these theories and study how stars shape their birth environment, but it's virtually impossible to use telescope observations of these clouds to separate the influence of the various processes, she said.

"That's why we need computer models," Offner explained.

After comparing models of clouds with gravity, magnetic fields, and stars, Offner noticed extra motions.

Her models showed that stellar winds interacting with the cloud magnetic field generated energy and influenced gas at far greater distances across the cloud than previously thought: These local magnetic fields caused action at a distance.

"Think of the magnetic fields like rubber bands that stretch across the cloud," Offner said.

"The winds push the field - it's like rubber bands being plucked. The waves outrun the wind and cause distant motions."

This research has implications for the tug-of-war between feedback - that is, the effect that the newly formed star has on its environment - and gravity on the scale of solar systems up to entire galaxies, Offner said.

As for the next step, Offner says she plans to study this process on larger scales, both in time and space. Her current study focused on one area within star-forming clouds; she said future studies will study the effects of magnetic fields and feedback on scales larger than a single cloud.

Stella Offner has written a blog post on this research for Nature.

Related Links
University of Texas at Austin
Stellar Chemistry, The Universe And All Within It

Tweet

Thanks for being there;
We need your help. The SpaceDaily news network continues to grow but revenues have never been harder to maintain.

With the rise of Ad Blockers, and Facebook - our traditional revenue sources via quality network advertising continues to decline. And unlike so many other news sites, we don't have a paywall - with those annoying usernames and passwords.

Our news coverage takes time and effort to publish 365 days a year.

If you find our news sites informative and useful then please consider becoming a regular supporter or for now make a one off contribution.

SpaceDaily Monthly Supporter
$5+ Billed Monthly

paypal only

SpaceDaily Contributor
$5 Billed Once

credit card or paypal

Falling stars hold clue for understanding dying stars
Tokyo, Japan (SPX) Sep 07, 2018
An international team of researchers has proposed a new method to investigate the inner workings of supernovae explosions. This new method uses meteorites and is unique in that it can determine the contribution from electron anti-neutrinos, enigmatic particles which can't be tracked through other means. Supernovae are important events in the evolution of stars and galaxies, but the details of how the explosions occur are still unknown. This research, led by Takehito Hayakawa, a visiting professor ... read more