The Environmental Dependence of Galaxy Properties in the Local Universe: Dependences on Luminosity, Local Density, and System Richness
The Environmental Dependence of Galaxy Properties in the Local Universe: Dependences on Luminosity, Local Density, and System Richness
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DOI:
10.1086/425529
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发表时间:
2004-11
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影响因子:
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通讯作者:
Masayuki Tanaka;T. Goto;S. Okamura;K. Shimasaku;J. Brinkmann
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文献类型:
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作者:
Masayuki Tanaka;T. Goto;S. Okamura;K. Shimasaku;J. Brinkmann
We investigate the environmental dependence of star formation and the morphology of galaxies in the local universe based on a volume-limited sample constructed from the data of the Sloan Digital Sky Survey. The sample galaxies (19,714 in total) are restricted to the redshift range of 0.030 200 km s-1 show no dependence on system richness, and most of the galaxies in those systems are non–star-forming early-type galaxies. Star formation activities of galaxies are different from those of field galaxies even in systems as poor as σ ∼ 100 km s-1. This result suggests that environmental mechanisms that are effective only in rich systems, such as ram pressure stripping of cold gas and harassment, have not played a major role in transforming galaxies into red early-type galaxies. Strangulation and interactions between galaxies, however, remain candidates of the driver of the environmental dependence. In the dense environment in the local universe, the slow transformation of faint galaxies occurs to some extent, but the transformation of bright galaxies is not clearly visible. We suggest that the evolution of bright galaxies is not strongly related to galaxy system, such as groups and clusters, while the evolution of faint galaxies is likely to be closely connected to galaxy system.