H I absorption in MHONGOOSE
Combined H I emission–absorption studies constrain the spin temperature and phase structure of the neutral atomic hydrogen interstellar medium (ISM). However, these studies have largely been limited to the Milky Way and the Local Group. We extend this technique to galaxies at distances of 7–22 Mpc u...
Gorde:
| Egile Nagusiak: | , , , , , , , , , |
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| Formatua: | Artigo |
| Hizkuntza: | Inglês |
| Argitaratua: |
EDP Sciences
2026-06-01
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| Saila: | Astronomy & Astrophysics |
| Gaiak: | |
| Sarrera elektronikoa: | https://www.aanda.org/articles/aa/full_html/2026/06/aa60207-26/aa60207-26.html |
| Etiketak: |
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