Formation and evolution of elliptical galaxies

By C. Chiosi, G. Carraro. 2002

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GCD+: a new chemodynamical approach to modelling supernovae and chemical enrichment in elliptical galaxies (2002, background): “Due to this expansion effect, the best model fails to explain the observed Kormendy relation, which is the same problem as that found in K01b (see also Chiosi & Carraro 2002).”
Stellar populations of early-type galaxies in different environments - II. Ages and metallicities (2006, background): “Chiosi & Carraro (2002) have recently build N-body-tree-SPH simulations incorporating cooling, star formation, energy feedback and chemical evolution.”
UV-Optical Colors as Probes of Early-Type Galaxy Evolution (2006, methodology): “Such a scenario can explain many of the observed properties of early-type galaxies, both at local and high redshift (Chiosi and Carraro 2002), without invoking hierarchical merger-driven processes (e.g. Toomre and Toomre 1972; Toomre 1977; Kauffmann et al. 1993; Somerville and Primack 1999; Benson…”
Feedback and metal enrichment in cosmological SPH simulations – II. A multiphase model with supernova energy feedback (2006, background): “…simulations assuming different types of initial conditions have also found such bursty behaviour for the star formation activity in small mass systems (e.g. Steinmetz & Navarro 1999; Carraro et al. 2001; Mayer et al. 2001; Pearce et al. 2001; Chiosi & Carraro 2002; Springel & Hernquist 2003).”