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...

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Hlavní autoři:	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
Médium:	Artigo
Jazyk:	Inglês
Vydáno:	IOP Publishing 2022-01-01
Edice:	The Astrophysical Journal Letters
Témata:	Astrochemistry Star formation Protostars Stellar winds Stellar jets Complex organic molecules
On-line přístup:	https://doi.org/10.3847/2041-8213/aca289
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