The dwarf galaxy population in Abell 2218
We present results from a deep photometric study of the rich galaxy cluster Abell 2218 (z = 0.18) based on archival Hubble Space Telescope WFPC2 F606W images. These have been used to derive the luminosity function to extremely faint limits (MF606W ≈ -13
|Collections||ANU Research Publications|
|Source:||Monthly Notices of the Royal Astronomical Society|
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