Physical Properties and H i-to-H2 Transition across Taurus Linear Edge

Physical Properties and H i-to-H2 Transition across Taurus Linear Edge

Studying the atomic-to-molecular transition is essential for understanding the evolution of the interstellar medium. The linear edge of the Taurus molecular cloud, clearly identified in the ^13 CO(1–0) intensity map, serves as an ideal site for investigating this transition. Utilizing the Arizona Ra...

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Bibliographic Details
Main Authors: Ningyu Tang, Feihang Miao, Gan Luo, Di Li, Junzhi Wang, Fujun Du, Donghong Wu, Shu Liu
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Interstellar medium
Online Access:https://doi.org/10.3847/1538-4357/adc686
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