ar X iv : 0 80 6 . 16 44 v 1 [ as tr o - ph ] 1 0 Ju n 20 08 A New Approach for Simulating Galaxy Cluster Properties

Abstract

We describe a subgrid model for including galaxies into hydrodynamical cos-mological simulations of galaxy cluster evolution. Each galaxy construct– or galcon– is modeled as a physically extended object within which star formation, galactic winds, and ram pressure stripping of gas are modeled analytically. Gal-cons are initialized at high redshift (z ∼ 3… (More)

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@inproceedings{ArieliarXI, title={ar X iv : 0 80 6 . 16 44 v 1 [ as tr o - ph ] 1 0 Ju n 20 08 A New Approach for Simulating Galaxy Cluster Properties}, author={Yinon Arieli and Yoel Rephaeli and Mark Norman} }