Mid-Infrared Evidence for Accelerated Evolution in Compact Group Galaxies

TL;DR

This study reveals that galaxies in Hickson compact groups exhibit a distinct bimodal mid-infrared color distribution, indicating accelerated evolution influenced by their dense environment, similar to the Coma infall region.

Contribution

It demonstrates that the unique MIR color distribution of HCG galaxies is environment-driven, highlighting accelerated galaxy evolution in compact groups compared to other environments.

Findings

HCG galaxies show a significant bimodal MIR color distribution.

The MIR gap in HCGs is statistically significant and not observed in other samples.

HCG galaxy evolution appears accelerated, resembling the Coma infall region environment.

Abstract

Compact galaxy groups are at the extremes of the group environment, with high number densities and low velocity dispersions that likely affect member galaxy evolution. To explore the impact of this environment in detail, we examine the distribution in the mid-infrared (MIR) 3.6-8.0 micron colorspace of 42 galaxies from 12 Hickson compact groups in comparison with several control samples, including the LVL+SINGS galaxies, interacting galaxies, and galaxies from the Coma Cluster. We find that the HCG galaxies are strongly bimodal, with statistically significant evidence for a gap in their distribution. In contrast, none of the other samples show such a marked gap, and only galaxies in the Coma infall region have a distribution that is statistically consistent with the HCGs in this parameter space. To further investigate the cause of the HCG gap, we compare the galaxy morphologies of the HCG and LVL+SINGS galaxies, and also probe the specific star formation rate (SSFR) of the HCG galaxies. While galaxy morphology in HCG galaxies is strongly linked to position with MIR colorspace, the more fundamental property appears to be the SSFR, or star formation rate normalized by stellar mass. We conclude that the unusual MIR color distribution of HCG galaxies is a direct product of their environment, which is most similar to that of the Coma infall region. In both cases, galaxy densities are high, but gas has not been fully processed or stripped. We speculate that the compact group environment fosters accelerated evolution of galaxies from star-forming and neutral gas-rich to quiescent and neutral gas-poor, leaving few members in the MIR gap at any time.