A serendipitous discovery of H i-rich galaxy groups with MeerKAT

Author:

Glowacki M1ORCID,Albrow L2,Reynolds T3ORCID,Elson E4ORCID,Mahony E K5ORCID,Allison J R6ORCID

Affiliation:

1. International Centre for Radio Astronomy Research (ICRAR), Curtin University , Bentley, WA 6102 , Australia

2. University of Canterbury, Department of Physics and Astronomy , Private Bag 4800, Christchurch 8020 , New Zealand

3. International Centre for Radio Astronomy Research (ICRAR), The University of Western Australia , 35 Stirling Hwy, Crawley, WA 6009 , Australia

4. Department of Physics & Astronomy, University of the Western Cape , Robert Sobukwe Rd, Bellville 7535 , South Africa

5. ATNF, CSIRO Space and Astronomy , PO Box 76, Epping, NSW 1710 , Australia

6. First Light Fusion Ltd , Unit 9/10 Oxford Pioneer Park, Mead Road, Yarnton, Kidlington OX5 1QU , UK

Abstract

ABSTRACT We report on the serendipitous discovery of 49 H i-rich galaxies in a 2.3 h Open Time observation with MeerKAT. We present their properties including their H i masses, intensity and velocity maps, and spectra. We determine that at least three H i-rich galaxy groups have been detected, potentially as part of a supergroup. Some members of these galaxy groups show clear interaction with each other in their H i emission. We cross-match the detections with PanSTARRS, Wide-field Infrared Survey Explorer, and Galaxy Evolution Explorer, and obtain stellar masses and star formation rates. One source is found to be a potential OH megamaser, but further follow-up is required to confidently determine this. For six sources with sufficient spatial resolution in H i, we produce rotation curves with BBarolo, generate mass models, and derive a dark matter halo mass. While the number of galaxies detected in this relatively short pointing appears to be at the high end of expectations compared to other MeerKAT observations and group H i mass function studies, this finding highlights the capability of MeerKAT for other serendipitous discoveries, and the potential for many more H i-rich galaxies to be revealed within both existing and upcoming Open Time data sets.

Funder

Australian Government

Australian Research Council

National Aeronautics and Space Administration

Jet Propulsion Laboratory

California Institute of Technology

Publisher

Oxford University Press (OUP)

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