Dynamical effects on galaxies in clusters

dc.creatorMoore, Ben
dc.creatorQuilis, Vicent
dc.creatorBower, Richard
dc.date2000-09-15
dc.date.accessioned2026-07-25T11:22:18Z
dc.descriptionThe observed morphological evolution since z ~ 0.5 within galaxy clusters provides evidence for a hierarchical universe. This evolution is driven by dynamical effects that operate within the cluster environment -- suppression of star-formation by ram-pressure and viscous stripping of the intra-galactic medium and tidal heating of disks by gravitational encounters.
dc.descriptionInvited review, XVth IAP meeting
dc.identifierhttps://arxiv.org/abs/astro-ph/0009248
dc.identifierhttp://arxiv.org/abs/astro-ph/0009248
dc.identifierASP Conf Ser Vol 197, eds Combes, Mamon and Charmandaris, 363
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/2182
dc.subjectAstrophysics
dc.titleDynamical effects on galaxies in clusters
dc.typetext

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