QR-Code

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...

Ausführliche Beschreibung

Gespeichert in:
Hauptverfasser: 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: Artigo
Sprache:Inglês
Veröffentlicht: IOP Publishing 2025-01-01
Schriftenreihe:The Astrophysical Journal Letters
Schlagworte:
Protoplanetary disks
Planet formation
Infrared spectroscopy
Circumstellar disks
Astrochemistry
Online-Zugang:https://doi.org/10.3847/2041-8213/adfbe3
Tags: Tag hinzufügen
Keine Tags, Fügen Sie das erste Tag hinzu!

Ähnliche Einträge