Large mirror polishing and figuring |
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| Authors: | W Scott Smith |
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| Institution: | (1) Department de Física de l'Atmosfera, Astronomia i Astrofisica, Universitat de Barcelona, Grup d'Astrofisica, Societat Catalana de Física del IEC, Barcelona, Spain |
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| Abstract: | The main purpose of this paper is to present a photometrical evolutionary model for galaxies belonging to rich clusters. This numerical code puts together both cluster dynamics and galaxy photometry in order to obtain theoretical predictions for galaxy evolution, directly comparable with observations. We have specially taken into account the galaxy-cluster interactions and the intrinsic galaxy evolution. |
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