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The radial distribution of H II regions in spiral galaxies · DOI 10.1086/160893

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astro-ph.CO 1 astro-ph.GA 1

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2026 2

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Resolved HI and Environmental Dynamics

astro-ph.GA · 2026-07-02 · unverdicted · novelty 2.0

SKA-mid AA4 will enable deep, spatially resolved HI imaging over hundreds of square degrees at column densities down to 10^18 cm^{-2} to study environmental gas processes from isolated galaxies to clusters.

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  • HI Simulations for Cosmology with the SKA Observatory astro-ph.CO · 2026-06-24 · unverdicted · none · ref 299

    Overview of HI modeling methods finds consistency in cosmic HI density but systematic differences in HI-halo mass relation shape and redshift evolution.