Environments of Galaxies: Stellar Mass and Color Dependence

Details Environments of Galaxies: Stellar Mass and Color Dependence Environments of Galaxies: Stellar Mass and Color Dependence

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..379..276b&link_type=abstract

Cosmic Frontiers ASP Conference Series, Vol. 379, proceedings of the conference held 31 July-4 August 2006 at Durham University,

Computer Science

Scientific paper

Environments for galaxies are measured using a projected neighborhood density Σ. Distributions in Σ for galaxies with different stellar masses are compared with the result for a random distribution. A detailed investigation of the fraction of red-sequence galaxies as a function of environment and stellar mass shows that there is a unified relation.

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