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In Cairns et al. (2019), we completed the first survey for molecular gas in galaxies located in Antlia, nearest merging galaxy cluster. Given its proximity, Antlia has rich multi-wavelength data which give us an unprecedented view on the interaction between the large-scale disturbed environment and the cluster galaxies. We found that galaxies in the Antlia cluster have surprisingly large molecular gas reservoirs, which could fuel and sustain high star formation and black hole activities. In the Antlia cluster, we might be seeing the intermediate step in the evolution of galaxies between fields and dense clusters, where the effects of the intracluster medium are just beginning to operate.

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