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

Published online by Cambridge University Press:  11 April 2023

C. Murugeshan Open the ORCID record for C. Murugeshan [Opens in a new window] ,
R. Džudžar ,
R. Bagge ,
T. O’Beirne ,
O. I. Wong Open the ORCID record for O. I. Wong [Opens in a new window] ,
V. A. Kilborn ,
M. E. Cluver ,
K. A. Lutz  and
A. Elagali
C. Murugeshan*
Affiliation:
ATNF, CSIRO, Space and Astronomy, PO Box 1130, Bentley, WA 6102, Australia
R. Džudžar
Affiliation:
Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia Tribalism PTY LTD, Lvl 1, 25 King Street, Melbourne, VIC 3000, Australia
R. Bagge
Affiliation:
School of Physics, The University of New South Wales, Kensington Campus, Old Main Building, Kensington, Sydney, NSW, Australia International Centre for Radio Astronomy Research, The University of Western Australia, 35 Stirling Highway, Crawley, WA 6009, Australia
T. O’Beirne
Affiliation:
ATNF, CSIRO, Space and Astronomy, PO Box 1130, Bentley, WA 6102, Australia International Centre for Radio Astronomy Research, The University of Western Australia, 35 Stirling Highway, Crawley, WA 6009, Australia
O. I. Wong
Affiliation:
ATNF, CSIRO, Space and Astronomy, PO Box 1130, Bentley, WA 6102, Australia International Centre for Radio Astronomy Research, The University of Western Australia, 35 Stirling Highway, Crawley, WA 6009, Australia
V. A. Kilborn
Affiliation:
Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Australia
M. E. Cluver
Affiliation:
Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia Department of Physics and Astronomy, University of the Western Cape, Robert Sobukwe Road, Bellville, 7535, South Africa
K. A. Lutz
Affiliation:
Observatoire Astronomique de Strasbourg, Université de Strasbourg, CNRS, UMR 7550, 67000 Strasbourg, France
A. Elagali
Affiliation:
Minderoo Foundation, 171 - 173 Mounts Bay Road, Perth, WA 6000, Australia School of Biological Sciences, The University of Western Australia, 35 Stirling Highway, Crawley, WA 6009, Australia
*
Corresponding author: C. Murugeshan, Email: chandrashekar.murugeshan@csiro.au.
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Abstract

We 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 ($\Omega_{\textrm{bar}}$) for a sub-sample of our galaxies and find that the values range from 10–90 $\textrm{km s}^{-1}$kpc$^{-1}$, in good agreement with previous studies.

Keywords

galaxies: evolutiongalaxies: fundamental parametersgalaxies: ISMgalaxies: kinematics and dynamics
Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 40 , 2023 , e018
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Copyright
© The Author(s), 2023. Published by Cambridge University Press on behalf of the Astronomical Society of Australia

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