The imacs cluster building survey. II. spectral evolution of galaxies in the epoch of cluster assembly

Abstract

The IMACS Cluster Building Survey (ICBS) provides spectra of ∼2200 galaxies 0.31 < z < 0.54 in five rich clusters (R ≲ 5 Mpc) and the field. Infalling, dynamically cold groups with tens of members account for approximately half of the supercluster population, contributing to a growth in cluster mass of ∼100% by the present day. The ICBS spectra distinguish non-star-forming (PAS) and poststarburst (PSB) from star-forming galaxies - continuously star-forming (CSF) or starbursts (SBH or SBO), identified by anomalously strong Hδ absorption or [O II] emission. For the infalling cluster groups and similar field groups, we find a correlation between PAS+PSB fraction and group mass, indicating substantial "preprocessing" through quenching mechanisms that can turn star-forming galaxies into passive galaxies without the unique environment of rich clusters. SBH + SBO starburst galaxies are common, and they maintain an approximately constant ratio (SBH+SBO)/CSF ≈ 25% in all environments - from field, to groups, to rich clusters. Similarly, while PSB galaxies strongly favor denser environments, PSB/PAS ≈ 10%-20% for all environments. This result, and their timescale τ ∼ 500 Myr, indicates that starbursts are not signatures of a quenching mechanism that produces the majority of passive galaxies. We suggest instead that starbursts and poststarbursts signal minor mergers and accretions, in star-forming and passive galaxies, respectively, and that the principal mechanisms for producing passive systems are (1) early major mergers, for elliptical galaxies, and (2) later, less violent processes - such as starvation and tidal stripping, for S0 galaxies. © 2013. The American Astronomical Society. All rights reserved.