MeerKAT-derived H I kinematics and the baryonic Tully–Fisher relation in the X-ray luminous cluster Abell 3408

dc.contributor.authorNdaliso, Xola
dc.contributor.authorBlecher, Tariq
dc.contributor.authorDeane, Roger
dc.contributor.authorElson, Ed
dc.date.accessioned2026-04-22T09:29:58Z
dc.date.available2026-04-22T09:29:58Z
dc.date.issued2025-09
dc.descriptionDATA AVAILABILITY : The MeerKAT reduced cubes and derived data products used in this work are available upon request from corresponding authors.
dc.description.abstractPlease read abstract in the article.
dc.description.departmentPhysics
dc.description.librarianam2026
dc.description.sdgNone
dc.description.sponsorshipFunding from the South African Radio Astronomy Observatory (SARAO), which is a facility of the National Research Foundation (NRF), an agency of the Department of Science and Innovation (DSI); funded by the South African Research Chairs Initiative of the DSI/NRF.
dc.description.urihttps://academic.oup.com/mnras
dc.identifier.citationNdaliso, X., Blecher, T., Deane, R.P. et al. 2025, 'MeerKAT-derived H I kinematics and the baryonic Tully–Fisher relation in the X-ray luminous cluster Abell 3408', Monthly Notices of the Royal Astronomical Society, 542, pp. 2167-2412. https://doi.org/10.1093/mnras/staf1376.
dc.identifier.issn0035-8711 (print)
dc.identifier.issn1365-2966 (online)
dc.identifier.other10.1093/mnras/staf1376
dc.identifier.urihttp://hdl.handle.net/2263/109698
dc.language.isoen
dc.publisherOxford University Press
dc.rights© The Author(s) 2025. This article is licensed under a Creative Commons Attribution 4.0 International License.
dc.subjectGalaxies: clusters: general
dc.subjectGalaxies: kinematics and dynamics
dc.subjectMeerKAT
dc.subjectSpace sustainability
dc.titleMeerKAT-derived H I kinematics and the baryonic Tully–Fisher relation in the X-ray luminous cluster Abell 3408
dc.typeArticle

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