Titlebook: Galaxy Evolution in Groups and Clusters; A JENAM 2002 Worksho Catarina Lobo,Margarida Serote Roos,Andrea Biviano Book 2003 Springer Science

官僚统治

Galaxy Evolution in Clusterss, perhaps because of the recent merging history of the clusters. We also present a recent analysis of population gradients in clusters which suggests that the observed evolution in cluster populations is consistent with a scenario where changing infall rates drive the fraction of star forming galax

处理

The Properties of the Galaxies in the Enacs Clusters, and the Relation Between Spirals and S0 Galaxithe early spirals (Sa-Sb), and the late spirals (including the emission-line galaxies). We also study the morphology-density relation, and we find that the segregation of the late spirals is driven mostly by global factors, while the segregation of Es, S0s and early spirals is driven mostly by local

吹牛大王

The Orbits of Cluster Galaxy Populations as Evolutionary Constraintsht ellipticals is probably affected by dissipative processes which invalidate the use of the collisionless Jeans equation. The equilibrium solution found for the early-spirals implies them to move on nearly-isotropic orbits. Late-spirals are instead found to be on mildly radial orbits, with the radi

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Buttress

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Dwarf LSB Galaxies and their Environment: The Virgo Cluster, The URSA Major Cluster, Isolated Galaxiy contribute significantly to the mass in galaxies if they have large mass-to-light ratios similar to those recently measured for Local Group dwarf galaxies..By a comparison with different environments, the Virgo Cluster seems to be highly ‘dwarf rich’ if considering the dwarf to giant ratio or its

FIR

Galaxy Threshing and Ultra-Compact Dwarfs in the Fornax Clusterture, the dwarf elliptical halo contents, up to 99% of the original dwarf luminosity, contribute a significant fraction of the populations of intergalactic stars, globulars, and gas in galaxy clusters.

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