Dust dynamics in disk dust traps and late planetesimal formation
Context. Streaming instability (SI) is currently the leading model for planetesimal formation in protoplanetary disks, but it typically operates on the radial drift timescale of solids toward the star, that is, within approximately the first million years. In the Solar System, however, some planetes...
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| Päätekijät: | , , |
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| Aineistotyyppi: | Artigo |
| Kieli: | Inglês |
| Julkaistu: |
EDP Sciences
2026-07-01
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| Sarja: | Astronomy & Astrophysics |
| Aiheet: | |
| Linkit: | https://www.aanda.org/articles/aa/full_html/2026/07/aa59196-26/aa59196-26.html |
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