CLASSY. XI. Tracing Neutral Gas Properties Using UV Absorption Lines and 21 cm Observations

CLASSY. XI. Tracing Neutral Gas Properties Using UV Absorption Lines and 21 cm Observations

Rest-frame far-ultraviolet (FUV) observations from JWST are revolutionizing our understanding of the high- z galaxies that drove reionization and the mechanisms by which they accomplished it. To fully interpret these observations, we must be able to diagnose how properties of the interstellar medium...

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Bibliographic Details
Main Authors: Kaelee S. Parker, Danielle A. Berg, Simon Gazagnes, John Chisholm, Bethan L. James, Matthew Hayes, Timothy Heckman, Alaina Henry, Michelle A. Berg, Karla Z. Arellano-Córdova, Xinfeng Xu, Dawn K. Erb, Crystal L. Martin, Weida Hu, Evan D. Skillman, Kristen B. W. McQuinn, Zuyi Chen, Dan P. Stark
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Galaxies
Ultraviolet spectroscopy
Interstellar line absorption
Lyman-alpha galaxies
High-redshift galaxies
Online Access:https://doi.org/10.3847/1538-4357/ad87cd
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https://doi.org/10.3847/1538-4357/ad87cd

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