Star formation near the Sun is driven by expansion of the Local Bubble

Catherine Zucker (), Alyssa A. Goodman, João Alves, Shmuel Bialy, Michael Foley, Joshua S. Speagle, Josefa Groβschedl, Douglas P. Finkbeiner, Andreas Burkert, Diana Khimey and Cameren Swiggum
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Catherine Zucker: Center for Astrophysics | Harvard & Smithsonian
Alyssa A. Goodman: Center for Astrophysics | Harvard & Smithsonian
João Alves: University of Vienna
Shmuel Bialy: Center for Astrophysics | Harvard & Smithsonian
Michael Foley: Center for Astrophysics | Harvard & Smithsonian
Joshua S. Speagle: University of Toronto
Josefa Groβschedl: University of Vienna
Douglas P. Finkbeiner: Center for Astrophysics | Harvard & Smithsonian
Andreas Burkert: University Observatory Munich
Diana Khimey: Center for Astrophysics | Harvard & Smithsonian
Cameren Swiggum: University of Vienna

Nature, 2022, vol. 601, issue 7893, 334-337

Abstract: Abstract For decades we have known that the Sun lies within the Local Bubble, a cavity of low-density, high-temperature plasma surrounded by a shell of cold, neutral gas and dust1–3. However, the precise shape and extent of this shell4,5, the impetus and timescale for its formation6,7, and its relationship to nearby star formation8 have remained uncertain, largely due to low-resolution models of the local interstellar medium. Here we report an analysis of the three-dimensional positions, shapes and motions of dense gas and young stars within 200 pc of the Sun, using new spatial9–11 and dynamical constraints12. We find that nearly all of the star-forming complexes in the solar vicinity lie on the surface of the Local Bubble and that their young stars show outward expansion mainly perpendicular to the bubble’s surface. Tracebacks of these young stars’ motions support a picture in which the origin of the Local Bubble was a burst of stellar birth and then death (supernovae) taking place near the bubble’s centre beginning approximately 14 Myr ago. The expansion of the Local Bubble created by the supernovae swept up the ambient interstellar medium into an extended shell that has now fragmented and collapsed into the most prominent nearby molecular clouds, in turn providing robust observational support for the theory of supernova-driven star formation.

Date: 2022
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DOI: 10.1038/s41586-021-04286-5

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