Wang, Jing, Lin, Xuchen, Liang, Ze-Zhong, de Blok, W. J. G. and van de Voort, Freeke ORCID: https://orcid.org/0000-0002-6301-638X
2026.
FEASTS and MHONGOOSE: H I column density distribution at z = 0 for N HI > 10 17.8 cm −2.
The Astrophysical Journal
1001
(1)
, 123.
10.3847/1538-4357/ae5178
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License URL: https://creativecommons.org/licenses/by/4.0/
Official URL: https://doi.org/10.3847/1538-4357/ae5178
Abstract
We present the first z = 0 H I column density distribution function, f(NHI), extending down to log(NHI/cm−2)=17.8 . This was derived from high-sensitivity 21 cm emission-line imaging at ∼1 kpc resolution. At high column densities (19.8 17.5 implies a covering fraction (fcov) of ∼0.7 within 1 kpc-scale H I-detected pixels at z = 0. Notably, for 17.817.8 gas within the virial radius around Milky Way–like galaxies. These findings provide new constraints on the baryonic flows and gaseous dynamics governing galaxy evolution.
| Item Type: | Article |
|---|---|
| Date Type: | Publication |
| Status: | Published |
| Schools: | Schools > Physics and Astronomy |
| Additional Information: | Full list of authors available at website: https://doi.org/10.3847/1538-4357/ae5178 License information from Publisher: LICENSE 1: URL: https://creativecommons.org/licenses/by/4.0/, Type: cc-by |
| Publisher: | American Astronomical Society |
| ISSN: | 0004-637X |
| Date of First Compliant Deposit: | 17 April 2026 |
| Date of Acceptance: | 27 February 2026 |
| Last Modified: | 17 Apr 2026 08:45 |
| URI: | https://orca.cardiff.ac.uk/id/eprint/186451 |
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