Tracing Pebble Drift History in Two Protoplanetary Disks with CO Enhancement

Pebble drift is an important mechanism for supplying the materials needed to build planets in the inner region of protoplanetary disks. Thus, constraining pebble drift’s timescales and mass flux is essential to understanding planet formation history. Current pebble drift models suggest pebble fluxes...

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Autors principals:	Tayt Armitage, Joe Williams, Ke Zhang, Sebastiaan Krijt, Leon Trapman, Richard A. Booth, Richard Teague, Charles J. Law, Chunhua Qi, David J. Wilner, Karin I. Öberg, Edwin A. Bergin, Sean M. Andrews, Romane Le Gal, Feng Long, Jane Huang, Jaehan Bae, Felipe Alarcón
Format:	Artigo
Idioma:	Inglês
Publicat:	IOP Publishing 2026-01-01
Col·lecció:	The Astrophysical Journal
Matèries:	Protoplanetary disks
Accés en línia:	https://doi.org/10.3847/1538-4357/ae353d
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