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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...

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Príomhchruthaitheoirí: de Blok W. J. G., Maccagni F. M., Chemin L., Haubner K., Morganti R., Oosterloo T. A., Kleiner D., Veronese S., Kurapati S., Healy J.
Formáid: Artigo
Teanga:Inglês
Foilsithe / Cruthaithe: EDP Sciences 2026-06-01
Sraith:Astronomy & Astrophysics
Ábhair:
Rochtain ar líne:https://www.aanda.org/articles/aa/full_html/2026/06/aa60207-26/aa60207-26.html
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