出版社:SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要:In this contribution the discovery and properties of ultra-compact dwarf galaxies are presented,
and their possible origin is discussed. This new type of galaxy resides in the cores of galaxy
clusters. In the fundamental plane diagram of stellar systems, the luminosity and kinematical
and structural properties of ultra-compact dwarfs locate them inbetween globular clusters and
small compact ellipticals (like M32). This regime would also be occupied by nuclei of dwarf
ellipticals if they were isolated from their galactic envelope or by the merger product of super
star-cluster complexes as they are found in strongly interacting galaxies. Future investigations of
ultra-compact dwarfs in different environments have to show which of these formation scenarios
is to be favoured.