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Icy Volatile Enhancements in Evolving Protoplanetary Disks

Protoplanetary disk ice lines shape a multitude of planet formation processes, setting the environmental composition through evolution. Ice line locations depend on molecular sublimation and deposition properties, but in dynamic disks where temperature and density structures change, so do the expect...

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Bibliografski detalji
Glavni autori: Elizabeth S. Yunerman, Ellen M. Price, Karin I. Öberg
Format: Artigo
Jezik:Inglês
Izdano: IOP Publishing 2026-01-01
Serija:The Astrophysical Journal
Teme:
Online pristup:https://doi.org/10.3847/1538-4357/ae60fe
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