Organic Chemistry in the H2-bearing, CO-rich Interstellar Ice Layer at Temperatures Relevant to Dense Cloud Interiors

Organic Chemistry in the H2-bearing, CO-rich Interstellar Ice Layer at Temperatures Relevant to Dense Cloud Interiors

Ice chemistry in the dense, cold interstellar medium (ISM) is probably responsible for the formation of interstellar complex organic molecules (COMs). Recent laboratory experiments performed at T ∼ 4 K have shown that irradiation of CO:N _2 ice samples analog to the CO-rich interstellar ice layer ca...

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Bibliographic Details
Main Authors: Rafael Martín-Doménech, Alexander DelFranco, Karin I. Öberg, Mahesh Rajappan
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Interstellar medium
Interstellar clouds
Interstellar molecules
Dense interstellar clouds
Ice composition
Complex organic molecules
Online Access:https://doi.org/10.3847/1538-4357/ad187e

Internet

https://doi.org/10.3847/1538-4357/ad187e

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