Paper:	Extremely Massive Clusters and their Link to Ultra Compact Dwarf Galaxies
Volume:	322, The Formation and Evolution of Massive Young Star Clusters
Page:	535
Authors:	Kissler-Patig, M.
Abstract:	In the following contribution I discuss the nature of the recently discovered extremely massive star clusters (106 to 108MSolar). How massive can a cluster get? When does it stop to be a classical globular cluster? I briefly discuss their link to other star clusters and in particular to Ultra Compact Dwarf Galaxies (the latter are argued to be neither Dwarf Galaxies nor Ultra Compact). I speculate on their nature as nuclear clusters that suffered accretion over their lifetime.

Astronomical Society of the Pacific
Conference Series

© Copyright 1988 - 2024 - Astronomical Society of the Pacific
No part of the material protected by this copyright may be reproduced or used in any form other than for personal use without written permission from the ASP.

Page generated in 0.066 seconds