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Talks in PDF





Name

Title

Link

S. Bardelli

The changing life of AGNs and their relationship with the feedback

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A. Biviano

A mid and far-IR view of the star formation activity in galaxy systems and their surroundings

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M. Bolzonella

The efficiency of galaxy formation in different environments

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R. Calvi

The morphology-mass relation in different environments at low redshift

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C. Chiosi

The Mass-Radius Plane of galaxies

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E. Corbelli

HeViCS and the path to star-formation in the cluster environment

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G. Cresci

Metallicity near and far

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O. Cucciati

The colour-density relation up to z=1.5: observations vs semianalytical models

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G. De Lucia

The environmental history of cluster galaxies in a LCDM Universe

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S. Di Serego

Dust and Gas in Early-Type Galaxies

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A. Gargiulo

Color gradients of early-type galaxies at 1<z<2

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P. Gavazzi

Environmental driven evolution of galaxies in the Great Wall

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A. Fritz

The evolution of early-type galaxies since z=1

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F. La Barbera

On the Radial Stellar Content of Early-type Galaxies

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A. Iovino

Introduction

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Y. Jaffe'

The effect of the environment on the gas and the stars of distant galaxies

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M. Mapelli

Life and death of ring galaxies

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E. Merlin

Simulating the formation and evolution of early-type galaxies

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P. Merluzzi

The quenching of star formation in a cluster population of dusty S0s

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P. Monaco

An internal driver for galaxy evolution to produce galaxy downsizing

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N. Napolitano

Dark to luminous mass fractions in early-type galaxies

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B. Poggianti

Conference Summary & Discussion

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V. Presotto

Color and mass segregation in zCOSMOS groups

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A. Raichoor

JKCS041: Evolution of galaxies in the richest environments at z~2.2

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G. Rodighiero

The dominant role of secular evolution at z~2

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M. Scodeggio

Exploring galaxy evolution with VIPERS Survey

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R. Sordo

Synthetic spectral libraries of stars and galaxies for Gaia mission

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M. Spavone

A new mechanism for the formation of wide disk-like polar rings

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C. Tortora

Dichotomy in galactic colour gradients

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B. Vulcani

The galaxy stellar mass function in different environments and its time evolution

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