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Fermi-LAT γ-Ray Study of the Interstellar Medium and Cosmic Rays in the Chamaeleon Molecular Cloud Complex: A Look at the Dark Gas as Optically Thick H i
Exploring the Properties of Warm and Cold Atomic Hydrogen in the Taurus and Gemini Regions
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Hard and bright gamma-ray emission at the base of the Fermi bubbles
The Search for Spatial Extension in High-latitude Sources Detected by the Fermi Large Area Telescope
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The XCO Conversion Factor from Galactic Multiphase ISM Simulations
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Optically Thick H i Does Not Dominate Dark Gas in the Local ISM
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Variations between Dust and Gas in the Diffuse Interstellar Medium. III. Changes in Dust Properties