Disciplines
Physics, Astronomy (100%)
Keywords
Cosmology,
Galaxies:formation,
Galaxies: evolution,
Galaxies: dwarfs,
Tidal interaction
Abstract
As a result of angular momentum and energy conservation gas-rich tidal arms are formed when two large galaxies
merge or closely interact. These tidal arms can fragment into a series of self-gravitating dwarf
galaxies. It is expected that the production of tidal-dwarf galaxies (TDGs) is more efficient in the cores of galaxy
clusters, due to the larger number of galaxy interactions. This project aims at investigating the chemical and
dynamical evolution of TDGs in different environments and compare the results with well-studied dwarf galaxies,
in order to investigate the nature of these object and, more in general, to study the role played by the environment
in the evolution of galaxies.
- Gerhard Hensler, Universität Kiel , associated research partner