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Talks in PDF





Name

Title

Link

S. Bardelli

The changing life of AGNs and their relationship with the feedback

A. Biviano

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

M. Bolzonella

The efficiency of galaxy formation in different environments

R. Calvi

The morphology-mass relation in different environments at low redshift

C. Chiosi

The Mass-Radius Plane of galaxies

E. Corbelli

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

G. Cresci

Metallicity near and far

O. Cucciati

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

G. De Lucia

The environmental history of cluster galaxies in a LCDM Universe

S. Di Serego

Dust and Gas in Early-Type Galaxies

A. Gargiulo

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

P. Gavazzi

Environmental driven evolution of galaxies in the Great Wall

A. Fritz

The evolution of early-type galaxies since z=1

F. La Barbera

On the Radial Stellar Content of Early-type Galaxies

A. Iovino

Introduction

Y. Jaffe'

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

M. Mapelli

Life and death of ring galaxies

E. Merlin

Simulating the formation and evolution of early-type galaxies

P. Merluzzi

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

P. Monaco

An internal driver for galaxy evolution to produce galaxy downsizing

N. Napolitano

Dark to luminous mass fractions in early-type galaxies

B. Poggianti

Conference Summary & Discussion

V. Presotto

Color and mass segregation in zCOSMOS groups

A. Raichoor

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

G. Rodighiero

The dominant role of secular evolution at z~2

M. Scodeggio

Exploring galaxy evolution with VIPERS Survey

R. Sordo

Synthetic spectral libraries of stars and galaxies for Gaia mission

M. Spavone

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

C. Tortora

Dichotomy in galactic colour gradients

B. Vulcani

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





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