An Ultraviolet Study of CO Chemistry in the Magellanic Clouds

How does molecular cloud chemistry change with metallicity? In this work, we study the relation between molecular hydrogen (H _2 ) and carbon monoxide (CO) at 1/2 and 1/5 solar metallicity using ultraviolet absorption spectroscopy obtained as part of the UV Legacy Library of Young Stars as Essential...

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Bibliographic Details
Main Authors: Kirill Tchernyshyov, Jessica K. Werk, Julia Roman-Duval
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astronomical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-3881/adf33a
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