Imprint of galaxy formation and evolution on globular cluster properties
Abstract
Description
We discuss the origin of physical properties of globular cluster systems (GCSs) in galaxies in terms of galaxy formation and evolution processes. Based on numerical simulations of dynamical evolution of GCSs in galaxies, we particularly discuss (1) the origin of radial density profiles of GCSs, (2) kinematics of GCSs in elliptical galaxies, (3) transformation from nucleated dwarf galaxies into GCs (e.g., omega Centauri), and (4) the origin of GCSs in the Large Magellanic Cloud (LMC).
8 pages, 4 figures, Conference proceedings for an invited talk at ESO conference ``Globular clusters - Guides to galaxies''
8 pages, 4 figures, Conference proceedings for an invited talk at ESO conference ``Globular clusters - Guides to galaxies''