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CORINOS. I. JWST/MIRI Spectroscopy and Imaging of a Class 0 Protostar IRAS 15398–3359

The origin of complex organic molecules (COMs) in young Class 0 protostars has been one of the major questions in astrochemistry and star formation. While COMs are thought to form on icy dust grains via gas-grain chemistry, observational constraints on their formation pathways have been limited to g...

Ausführliche Beschreibung

Gespeichert in:
Hauptverfasser: Yao-Lun Yang, Joel D. Green, Klaus M. Pontoppidan, Jennifer B. Bergner, L. Ilsedore Cleeves, Neal J. Evans II, Robin T. Garrod, Miwha Jin, Chul Hwan Kim, Jaeyeong Kim, Jeong-Eun Lee, Nami Sakai, Christopher N. Shingledecker, Brielle Shope, John J. Tobin, Ewine F. van Dishoeck
Format: Artigo
Sprache:Inglês
Veröffentlicht: IOP Publishing 2022-01-01
Schriftenreihe:The Astrophysical Journal Letters
Schlagworte:
Astrochemistry
Star formation
Protostars
Stellar winds
Stellar jets
Complex organic molecules
Online-Zugang:https://doi.org/10.3847/2041-8213/aca289
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