We examine the ultraviolet and optical colours of 906 cluster galaxies from the KASI-Yonsei Deep Imaging Survey of Clusters (KYDISC). The sample has 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.
|Number of pages||12|
|Journal||Monthly Notices of the Royal Astronomical Society|
|Publication status||Published - 2019 Sept 21|
Bibliographical noteFunding Information:
Parts of this research were conducted by the Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), through project number CE170100013. SKY acknowledges support from the Korean National Research Foundation (2017R1A2A1A05001116). As the PI of the KYDISC project, SKY acted as a corresponding author. MK was supported by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (No. 2017R1C1B2002879). YKS acknowledges support from the National Research Foundation of Korea (NRF) grant funded by the Ministry of Science and ICT (No. 2019R1C1C1010279). LCH was supported by the National Key R&D Program of China (2016YFA0400702) and the National Science Foundation of China (11721303). SO thanks DL for the consistent support.
© 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science