Impact of Galaxy Mergers on the Colours of Cluster Galaxies

• Published in: arXiv.org 2019-07
• Main Authors: Oh, Sree, Kim, Keunho, Lee, Joon Hyeop, Kim, Minjin, Yun-Kyeong Sheen, Rhee, Jinsu, Ree, Chang H, Jeong, Hyunjin, Ho, Luis C, Jaemann Kyeong, Park, Byeong-Gon, Yi, Sukyoung K
• Format: Article
• Language: English
• Subjects: Deposition; Galactic clusters; Galaxies; Galaxy mergers & collisions; Morphology; Quenching; Signatures; Star & galaxy formation; Star clusters; Star formation
• ISSN: 2331-8422
• DOI: 10.48550/arxiv.1907.04858

We examine the ultraviolet and optical colours of 906 cluster galaxies from the KASI-Yonsei Deep Imaging Survey of Clusters (KYDISC). Galaxies have been divided into two categories, morphologically-disturbed and undisturbed galaxies, based on the visual signatures related to recent mergers. We find that galaxies with signatures of recent mergers show significantly bluer colours than undisturbed galaxies. Disturbed galaxies populate more on the cluster outskirts, suggesting recent accretion into the cluster environment, which implies that disturbed galaxies can be less influenced by the environmental quenching process and remain blue. However, we still detect bluer colours of disturbed galaxies in all locations (cluster core and outskirts) for the fixed morphology, which is difficult to understand just considering the difference in time since infall into a cluster. Moreover, blue disturbed galaxies show features seemingly related to recent star formation. Therefore, we suspect that mergers make disturbed galaxies keep their blue colour longer than undisturbed galaxies under the effect of the environmental quenching through either merger-induced star formation or central gas concentration which is less vulnerable for gas stripping.