Show simple item record

dc.contributor.authorCluver, M.E.
dc.contributor.authorMurugeshan, C.
dc.contributor.authorDžudžar, R.
dc.date.accessioned2024-02-14T09:12:46Z
dc.date.available2024-02-14T09:12:46Z
dc.date.issued2023
dc.identifier.citationMurphy, K., Berk, J., Muhwava-Mbabala, L., Booley, S., Harbron, J., Ware, L., Norris, S., Zarowsky, C., Lambert, E.V. and Levitt, N.S., 2023. Using the COM-B model and Behaviour Change Wheel to develop a theory and evidence-based intervention for women with gestational diabetes (IINDIAGO). BMC Public Health, 23(1), p.894.en_US
dc.identifier.issn13233580
dc.identifier.urihttp://dx.doi.org/10.1017/pasa.2023.19
dc.identifier.urihttp://hdl.handle.net/10566/9299
dc.description.abstractWe present a new high-resolution neutral atomic hydrogen (Hi) survey of ring galaxies using the Australia Telescope Compact Array (ATCA). We target a sample of 24 ring galaxies from the Buta (1995) Southern Ring Galaxy Survey Catalogue in order to study the origin of resonance-, collisional- and interaction-driven ring galaxies. In this work, we present an overview of the sample and study their global and resolved Hi properties. In addition, we also probe their star formation properties by measuring their star formation rates (SFR) and their resolved SFR surface density profiles. We find that a majority of the barred galaxies in our sample are Hi-deficient, alluding to the effects of the bar in driving their Hi deficiency. Furthermore, for the secularly evolving barred ring galaxies in our sample, we apply Lindblad's resonance theory to predict the location of the resonance rings and find very good agreement between predictions and observations. We identify rings of Hi gas and/or star formation co-located at one or the other major resonances. Lastly, we measure the bar pattern speed for a sub-sample of our galaxies and find that the values range from 10-90 kpc, in good agreement with previous studies. © 2023 The Author(s). Published by Cambridge University Press on behalf of the Astronomical Society of Australia.en_US
dc.language.isoenen_US
dc.publisherCambridge University Pressen_US
dc.subjectevolutionen_US
dc.subjectfundamental parametersen_US
dc.subjectkinematicsen_US
dc.subjectdynamicsen_US
dc.subjectgalaxiesen_US
dc.titleThe h i in ring galaxies survey (h i -rings) - effects of the bar on the h i gas in ring galaxiesen_US
dc.typeArticleen_US


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record