Cosmic Cascades: How Disk Substructure Regulates the Flow of Water to Inner Planetary Systems

The influx of icy pebbles to the inner regions of protoplanetary disks constitutes a fundamental ingredient in most planet formation theories. The observational determination of the magnitude of this pebble flux and its dependence on disk substructure (disk gaps as pebble traps) would be a significa...

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Bibliographic Details

Published in:	The Astrophysical Journal Letters
Main Authors:	Sebastiaan Krijt, Andrea Banzatti, Ke Zhang, Paola Pinilla, Till Kaeufer, Edwin A. Bergin, Colette Salyk, Klaus Pontoppidan, Geoffrey A. Blake, Feng Long, Jane Huang, María José Colmenares, Joe Williams, Adrien Houge, Mayank Narang, Miguel Vioque, Michiel Lambrechts, L. Ilsedore Cleeves, Karin Öberg, The JDISCS Collaboration
Format:	Article
Language:	English
Published:	IOP Publishing 2025-01-01
Subjects:	Protoplanetary disks Planet formation Infrared spectroscopy Circumstellar disks Astrochemistry
Online Access:	https://doi.org/10.3847/2041-8213/adfbe3