The H i in Ring Galaxies Survey (H i-RINGS) - Effects of the bar on the H i gas in ring galaxies

Abstract We present a new high-resolution neutral atomic hydrogen (H i ) 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 H i 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 H i deficient, alluding to the effects of the bar in driving their H i 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 H i gas and/or star formation co-located at one or the other major resonances. Lastly, we measure the bar pattern speed (Ω bar ) for a sub-sample of our galaxies and find that the values range from 10 – 90 km s −1 kpc −1 , in good agreement with previous studies.