Recent Results on Star Clusters in Galaxy Nuclei
Recent surveys have revealed that a large fraction of galaxies host compact star clusters in their centers. These sources trace dissipational processes that generate mass concentrations in galaxy nuclei, and represent a possible vehicle for creation of "seed" black holes that are the precursors for luminous accreting systems. This talk will summarize recent observations bearing on the stellar content of nuclear star clusters, and possible connections to galaxy bulges and central black holes.
