| dc.contributor.author | Namumba, Brenda | |
| dc.contributor.author | Román, Javier | |
| dc.contributor.author | Jarvis, Matt | |
| dc.date.accessioned | 2023-05-09T07:22:39Z | |
| dc.date.available | 2023-05-09T07:22:39Z | |
| dc.date.issued | 2023 | |
| dc.identifier.citation | Namumba, B. et al. (2023). Mightee-h i: Possible interactions with the galaxy NGC 895. Monthly Notices of the Royal Astronomical Society, 521(4), 5177-5190. 10.1093/mnras/stad857 | en_US |
| dc.identifier.issn | 1365-2966 | |
| dc.identifier.uri | 10.1093/mnras/stad857 | |
| dc.identifier.uri | http://hdl.handle.net/10566/8903 | |
| dc.description.abstract | The transformation and evolution of a galaxy is strongly influenced by interactions with its environment. Neutral hydrogen (H i) is an excellent way to trace these interactions. Here, we present H i observations of the spiral galaxy NGC 895, which was previously thought to be isolated. High-sensitivity H i observations from the MeerKAT large survey project MIGHTEE reveal possible interaction features, such as extended spiral arms and the two newly discovered H i companions, that drive us to change the narrative that it is an isolated galaxy. We combine these observations with deep optical images from the Hyper Suprime Camera to show an absence of tidal debris between NGC 895 and its companions. | en_US |
| dc.language.iso | en | en_US |
| dc.publisher | Oxford University Press | en_US |
| dc.subject | Astronomy | en_US |
| dc.subject | Physics | en_US |
| dc.subject | Galaxies | en_US |
| dc.subject | Digital storage | en_US |
| dc.subject | Astrophysics | en_US |
| dc.title | Mightee-h i: Possible interactions with the galaxy NGC 895 | en_US |
| dc.type | Article | en_US |
