期刊
ASTROPHYSICAL JOURNAL
卷 770, 期 1, 页码 -出版社
IOP PUBLISHING LTD
DOI: 10.1088/0004-637X/770/1/62
关键词
galaxies: clusters: general; galaxies: evolution; galaxies: groups: general; galaxies: high-redshift; galaxies: star formation; galaxies: stellar content
资金
- NSF [AST-0407343]
- NASA through NASA-JPL [1310394]
- ASI [I/016/07/0]
- ASI-INAF [I/009/10/0]
- Research Corporation through a Cottrell Scholars Award
The IMACS Cluster Building Survey (ICBS) provides spectra of similar to 2200 galaxies 0.31 < z < 0.54 in five rich clusters (R less than or similar to 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 similar to 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 H delta 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 approximate to 25% in all environments-from field, to groups, to rich clusters. Similarly, while PSB galaxies strongly favor denser environments, PSB/PAS approximate to 10%-20% for all environments. This result, and their timescale tau similar to 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.
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