Astronomy and Astrophysics – Astrophysics
Scientific paper
2005-11-30
Astronomy and Astrophysics
Astrophysics
Submitted to ApJ
Scientific paper
We investigate the extent to which galaxies' star-formation histories and morphologies are determined by their clustocentric distance and their nearest cluster's richness. We look at three tracers of star-formation history (i-band absolute magnitude M_i, [g-r] color, and Halpha emission line equivalent width) and two indicators of galaxy morphology (surface brightness and radial concentration) for 52,569 galaxies in the redshift range of 0.015
Berlind Andreas A.
Blanton Michael R.
Hogg David Wardell
Quintero Alejandro D.
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