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...

詳細記述

書誌詳細
出版年:The Astronomical Journal
主要な著者: Kirill Tchernyshyov, Jessica K. Werk, Julia Roman-Duval
フォーマット: 論文
言語:英語
出版事項: IOP Publishing 2025-01-01
主題:
オンライン・アクセス:https://doi.org/10.3847/1538-3881/adf33a

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