MeerKAT-64 discovers wide-spread tidal debris in the nearby NGC 7232 galaxy group
Brenda Namumba, Baerbel Silvia Koribalski, Gyula I. G. J\'ozsa, Karen, Lee-Waddell, Michael Gordon Jones, Claude Carignan, Lourdes, Verdes-Montenegro, Roger Ianjamasimanana, Erwin W.J.G. de Blok, Michelle, Cluver, Julian Garrido, Susana Sanchez-Exposito, Athanaseus Ramaila

TL;DR
This paper reports the discovery of extensive, previously undetected cold neutral hydrogen tidal debris around the NGC 7232 galaxy group using MeerKAT, revealing complex gas structures and interactions.
Contribution
First high-resolution MeerKAT observations uncover large-scale extsc{HI} streams and debris in the NGC 7232 group, providing new insights into galaxy interactions and gas dynamics.
Findings
extsc{HI} streams extend over 140 kpc, three times the galaxy triplet's size.
The extsc{HI} debris mass is about 6.6 billion solar masses, over half of the triplet's total extsc{HI}.
NGC 7232 and NGC 7233 are extsc{HI} deficient, indicating ongoing interactions.
Abstract
We report the discovery of large amounts of previously undetected cold neutral atomic hydrogen (\HI) around the core triplet galaxies in the nearby NGC~7232 galaxy group with MeerKAT. With a physical resolution of 1 kpc, we detect a complex web of low surface brightness \HI\ emission down to a 4 column density level of 1 10 cm (over 44 \kms ). The newly discovered H\,{\sc i} streams extend over 20 arcmin corresponding to 140~kpc in projection. This is 3 times the \HI\ extent of the galaxy triplet (52 kpc). The \HI\ debris has an \HI\ mass of 6.6 ~M, more than 50\% of the total \HI\ mass of the triplet. Within the galaxy triplet, NGC~7233 and NGC~7232 have lost a significant amount of \HI\ while NGC~7232B appears to have an excess of \HI. The \HI\ deficiency in NGC~7232 and NGC~7233 indicates that…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
