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

@article{Zucker2022StarFN,
  title={Star formation near the Sun is driven by expansion of the Local Bubble},
  author={Catherine Zucker and Alyssa A. Goodman and Jo{\~a}o Alves and Shmuel Bialy and Michael M. Foley and Joshua S. Speagle and Josefa Gro$\beta$schedl and Douglas P. Finkbeiner and Andreas Burkert and Diana Khimey and Cameren N. Swiggum},
  journal={Nature},
  year={2022},
  volume={601},
  pages={334-337}
}
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 dust 1 – 3 . However, the precise shape and extent of this shell 4 , 5 , the impetus and timescale for its formation 6 , 7 , and its relationship to nearby star formation 8 have remained uncertain, largely due to low-resolution models of the local interstellar medium. Here we report an analysis of the three-dimensional positions… 
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