Rice astronomer helps find evidence of an accretion disk around a young star outside the Milky Way
Astronomers have uncovered evidence of a rotating disc of material circling a massive young star in a nearby galaxy for the first time. Megan Reiter, assistant professor of physics and astronomy at Rice University, was part of the team of researchers who announced their discovery in a study published in Nature.
“This is strong evidence that high-mass stars, which are several times bigger than the Sun, form in the same way as lower-mass stars,” Reiter said. “That’s been a big question for a long time.”
Located in a galaxy neighboring the Milky Way called the Large Magellanic Cloud, the disc-sporting star was first discovered thanks to a protostellar jet ⎯ a signature feature of forming stars.
“As a star forms, the cloud of surrounding matter collapses, forming a disc,” Reiter said. “The disc feeds material onto the star, which will throw away about 1-10% of it into these big bipolar jets. These jets can be quite large, so they’re easy to spot. Because they are shot out as part of this accretion process, the jets are also a bit of a history record that can tell you something about how the star is putting itself together.”
The jet was first spotted using the Multi Unit Spectroscopic Explorer instrument on the European Southern Observatory’s Very Large Telescope.
“After we saw the jet, the natural next thing to say is, well, these jets have to come from a disc ⎯ there must be a disc around that star,” Reiter said.
To test this hypothesis, the team used the Atacama Large Millimeter/submillimeter Array (ALMA) in Chile to collect data on the fledgling star and its surroundings.
“Trying to spot a disk around a high-mass star is challenging, not least because it’s a relatively short-lived phenomenon,” Reiter said, explaining that a low-mass star like the Sun ⎯ with an approximate lifespan of 10 billion years ⎯ would only sport a disc for 3-10 million years during its formation.
Moreover, at least in the Milky Way, the stardust swirling around high-mass stars tends to shroud their surroundings from view, making it difficult to observe a disc taking shape. Thankfully, visibility is much better in the Large Magellanic Cloud, where star-forming matter is different.
“It’s arguably more exciting to discover a disc in this neighboring galaxy as opposed to our own, because the conditions there are closer to what we think things were like earlier in the universe,” Reiter said. “It’s like we’re getting a window into how stars formed earlier on in the evolution of the universe.”
Anna McLeod, an associate professor at Durham University in the U.K. and lead author of the study, said that upon seeing evidence for a rotating structure in the ALMA data, she and her team could scarcely believe they had detected the first extragalactic accretion disc.
“It was a special moment,” McLeod said. “We know discs are vital to forming stars and planets in our galaxy, and here for the first time we’re seeing direct evidence for this in another galaxy.”
For more on this discovery:
- Astronomers Uncover a Planet-Forming Disc in Another Galaxy
- First-Ever Circumstellar Disc Discovered Beyond the Milky Way
Reference: “A probable Keplerian disk feeding an optically revealed massive young star” by Anna F. McLeod, Pamela D. Klaassen, Megan Reiter, Jonathan Henshaw, Rolf Kuiper and Adam Ginsburg, 29 November 2023, Nature.
DOI: 10.1038/s41586-023-06790-2
The research was supported by the Royal Society (URF/R1/221620), the German Research Foundation (KU 2849/9) and the National Science Foundation (2008101, 2206511, 2142300).