3-D Views of Interstellar Supernova “Cavities” Reveal Explosive Star-forming Regions

Orion Nebula

 

“3D data will revolutionize our understanding of star formation in our galaxy by allowing us to chart where stars fall in relation to dense gas,” wrote Harvard astrophysicist Michael Foley in an email to The Daily Galaxy. “By doing so, we can study a number of outstanding questions, such as how stellar feedback (the ways in which stars affect their environments throughout their lives) either inhibits or promotes new star formation. Using 3D data, we have found that many famous star-forming regions in our solar neighborhood, such as Orion, fall on the edges of bubbles of gas and dust swept up by supernova explosions. 

“These findings,” continued Foley, “suggest that supernovae may play a large role in creating the proper conditions for new stars to be born. By studying more regions in 3D, we can determine how common this process is and how it affects other properties of stars. For example, how do stars produced in this way inherit elements created in supernova explosions? Might the explosions affect the kinematics of nearby stars? With 3D data, we are at the cusp of finally being able to  tackle some of these fascinating questions.”

It seems clear that we are going to see a ‘swiss cheese’ picture of the interstellar medium, with stars forming at the edge of the holes, as we map more and more of the galaxy”

Highest-resolution 3D view

Astronomers studying the structure of the Milky Way galaxy have released the highest-resolution 3D view of the Orion star-forming region. The image and interactive figure were presented today at a press conference hosted by the American Astronomical Society. Led by researchers at the Center for Astrophysics | Harvard & Smithsonian, the work connects 3D data on young stars and interstellar gas around the Orion complex of star-forming regions. Analysis of the 2D and 3D images, alongside theoretical modeling, shows that supernova explosions within the last 4 million years produced large cavities in the interstellar material associated with Orion.

One particular cavity the team discovered may help explain the origin of Barnard’s Loop, a famous and mysterious semi-circle in the night sky first observed in 1894.

The study relies on 3D positions and velocities for young stars and interstellar clouds obtained using Gaia, a space telescope run by the European Space Agency. The team combined the Gaia-derived 3D data with existing 2D observations of the Orion region to piece together its star-formation history.

Orion Nebula

“Our first large-scale 3D look at Orion tells us so much,” says Foley at the Center for Astrophysics (CfA) who led the study. “Prior to this work, most studies of Orion were confined to two dimensions—up-down and left-right on the sky. By adding in the third dimension—distance—we can begin to map out all sorts of interesting structures, like huge cavities of gas and dust or clusters of stars with very interesting motions. Combining the information from the interstellar gas and stars leads us to believe cavities were produced by a number of supernovae over the last few million years.”

“Orion has had quite an exciting history,” he adds.

One or more supernovae, played a large role in the formation of Barnard’s Loop

One of the cavities detected by the team appears to correspond with Barnard’s Loop, a famous, giant arc of hot gas in the Orion region that astronomers have studied for over a hundred years. The origin of the arc is debated, but the new study offers evidence that a certain cluster of stars, which produced one or more supernovae, played a very large role in the formation of Barnard’s Loop.

Most of the new star formation in the Orion complex appears to happen on the edges of the giant cavities—one of which is nearly 500 light years wide—that appear throughout the region, suggesting that the supernovae that formed the cavities are ultimately responsible for the formation of the next generation of stars.

The new findings are consistent with the team’s previous work on the Per-Tau Supershell Local Bubble around the Sun.

Supernova explosions create conditions ripe for the formation of new stars

“It seems clear that we are going to see a ‘swiss cheese’ picture of the interstellar medium, with stars forming at the edge of the holes, as we map more and more of the galaxy,” says Alyssa Goodman, Harvard professor, CfA astronomer and co-author on the study.

“We believe that shells and loops in Orion, the Per-Tau shell, and the Local Bubble are the first of many discoveries relating new star formation to old supernovae,” Foley says. “Supernovae sweep up gas and dust into dense clumps, leading to the perfect birthplaces for new stars. The Orion region, rich in both star formation and supernovae, is the latest example of that.”

The new Orion results support the theory that when massive stars end their lives as supernova explosions, they create conditions ripe for the formation of new stars. The team is hard at work analyzing other regions in the Milky Way galaxy in 3D, and using numerical simulations, to see just how common supernova-driven star formation really is.

“Thanks to the work of many incredible scientists, 3D data will transform our understanding of star formation in our galaxy,” Foley notes. “It may be much more explosive than we even imagine!”

Soon all scientists will explore their ‘universes’ in 3D”

The scholarly paper presenting the Orion work contains 3D interactive figures showcasing the findings, as do essentially all of this team’s recent publications. The team’s interactive figures, which have appeared over the past few years in Nature, The Astrophysical Journal, and The Astrophysical Journal Letters, were produced using the “glue” visualization software created by NASA in-part to explore incoming data from the James Webb Space Telescope.

The figures make use of a plug-in for glue, written by co-author Catherine Zucker of the Space Telescope Science Institute, to export any author’s figures to an interactive graphing environment. The plug-in allows authors to manipulate figures in an ordinary web browser and explore their data further.

Use of the open-source glue software, and web versions of it, are currently making their way from astronomy to other areas of science. Goodman, the founder of glue, hopes that, “soon all scientists will explore their ‘universes’ in 3D, and share findings in publications just as easily as astronomers can today.”

More information: Michael Foley et al, A 3D View of Orion: I. Barnard’s Loop, Authorea (2022).

Image credit top of page: Orion Nebula

Michael Foley and Harvard CfA

 

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