Main sequence of star formation and colour bimodality considering galaxy environment
arXiv:2405.00481 · doi:10.1016/j.dark.2024.101802
Abstract
This study involves the use of friend-of-friend method on the volume limited samples constructed from the Sloan Digital Sky Survey Data Release 12 (SDSS DR12) to classify the galaxies into isolated and non-isolated environments hence to investigate the influence of the galaxy environment on the main sequence of star formation, and colour bimodality. We classified the galaxies into the luminous volume-limited sample with (mag), and the faint volume-limited sample with (mag). Using the WHAN diagnostic diagram we assignedthe samples into star-forming, strong AGN, weak AGN, and retired galaxies based on their environment (isolated and non-isolated). The friend-of-friend method was successful in producing consistent results regarding the stellar mass-SFR and stellar mass-colour known relations. Apart from that the decrease in the slope of the main sequence for star-forming galaxies by dex and intercept by dex for the luminous sample was observed while the faint sample a decrease of dex in slope and dex in intercept was observed between isolated and non-isolated galaxies. A significant difference on the number of galaxies between isolated and non-isolated galaxies within, above and below the main sequence by , , for the luminous sample while for the faint sample by , , on average, respectively are observed. A significant difference in the number of galaxies in the blue cloud, green valley, and red sequence by , , for luminous sample while for faint sample by , , on average, respectively was observed. The study concludes that the galaxy environment influences the shaping and positioning of galaxies along the star formation main sequence and colour bimodality.
arXiv comment14 pages, 3 figures
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