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

Autor(en)

Catherine Zucker, Alyssa A. Goodman, João Alves, Shmuel Bialy, Michael Foley, Joshua S. Speagle, Josefa Großschedl, Douglas P. Finkbeiner, Andreas Burkert, Diana Khimey, Cameren Swiggum

Abstrakt

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 dust1,2,3. 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 spatial9,10,11 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.

Organisation(en)

Institut für Astrophysik

Externe Organisation(en)

Harvard-Smithsonian Center for Astrophysics, Space Telescope Science Institute, University of Maryland, College Park, University of Toronto, Harvard University, Universitäts-Sternwarte München, Max-Planck-Institut für extraterrestrische Physik, University of Wisconsin, Madison

Journal

Nature

Band

601

Seiten

334–337

Anzahl der Seiten

4

ISSN

0028-0836

DOI

https://doi.org/10.1038/s41586-021-04286-5

Publikationsdatum

01-2022

Peer-reviewed

Ja

ÖFOS 2012

103004 Astrophysik, 103003 Astronomie

Schlagwörter

Link zum Portal

https://ucrisportal.univie.ac.at/de/publications/225bcb34-71c7-43dc-bbe2-0178810796c9