Stellar Outbursts and Chondrite Composition
The temperatures of observed protoplanetary disks are not sufficiently high to produce the accretion rate needed to form stars, nor are they sufficient to explain the volatile depletion patterns in CM, CO, and CV chondrites and terrestrial planets. We revisit the role that stellar outbursts, caused...
| Główni autorzy: | , , , , , |
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| Format: | Artykuł |
| Język: | English |
| Wydane: |
IOP Publishing
2023-01-01
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| Seria: | The Astrophysical Journal |
| Hasła przedmiotowe: | |
| Dostęp online: | https://doi.org/10.3847/1538-4357/acfb02 |