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Titlebook: Environment and the Formation of Galaxies: 30 years later; Proceedings of Sympo Ignacio Ferreras,Anna Pasquali Conference proceedings 2011

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The Symbiotic Relationship Between the Evolution of Galaxy Groups and Their Resident Galaxies,ediate environment rather than in larger clusters. We report on observational and analytical work that shows how the evolution of the group environment influences the evolution of the resident galaxies and how feedback resulting from the evolution of individual galaxies influences their larger envir
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The Fundamental Plane of Early-Type Galaxies: Environmental Dependence from , Through ,, (ETGs) in the optical (griz) and Near-Infrared (YJHK) wavebands. The intercept “.” of the FP decreases from high- to low-density regions, implying that galaxies at low density have on average lower mass-to-light ratios than their high-density counterparts. Since the variation of “.” is the same at
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,On Galaxy Mass–Radius Relationship,on follows about the observed relationship between stellar mass and effective radius, .. − .., for early type galaxies (ETGs). The key of this correlation lies in the deep link which has to exist between cosmology and the existence of the FP. The general strategy consists in using the two-component
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Wundballistik -- Grundlagen und AnwendungenUsing data from our Parkes and ATCA . survey of six groups analogous to the Local Group, we find that the . mass function and velocity distribution function for loose groups are the same as those for the Local Group. Both mass functions confirm that the “missing satellite” problem exists in other galaxy groups.
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