Crete, 1/24 Mapping the kinematics and stellar populations of E/S0s with SAURON Harald Kuntschner Crete, 12 th August 2004.
Dec. 1-8, 2010 DARK MATTER IN GALAXIES Alessandro Romeo Onsala Space Observatory Chalmers University of Technology SE-43992 Onsala, Sweden.
Mariangela Bernardi UPitt/UPenn Galaxies Properties in the SDSS: Evolution, Environment and Mass Galaxies Properties in the SDSS: Evolution, Environment.
P. Saracco 1 M. Longhetti 1, A. Gargiulo 1 1 INAF – Osservatorio Astronomico di Brera, Milano Italy Galaxy Evolution and Environment - Bologna, November.
Dark Matter and Galaxy Formation Section 4: Semi-Analytic Models of Galaxy Formation Joel R. Primack 2009, eprint arXiv:0909.2021 Presented by: Michael.
THE BUILD-UP OF THE COLOUR-MAGNITUDE RELATION IN LOW-Z GALAXY CLUSTERS
The nuclear activity of late-type galaxies in the Virgo Cluster
Unravelling the formation and evolutionary histories of the most massive galaxies Ilani Loubser (Univ. of the Western Cape)
Massive galaxies at z ~ 2 from K20+
The Sino-French IFU Workshop ---Lijing PU,SHIBI ([email protected]; [email protected])[email protected]@ynao.ac.cn --Yunnan Observatory (Group.
Mapping the kinematics and stellar populations of E/S0s with SAURON
Center for Astronomy. Vision & Objectives Maintain the number 1 status in Korea. Aim to be a world-class astronomy institute. Regarding Yonsei-Oxford.
