Paper:	Cluster Disruption: Combining Theory and Observations
Volume:	388, Mass Loss from Stars and the Evolution of Stellar Clusters
Page:	353
Authors:	Bastian, N.; Gieles, M.
Abstract:	We review the theory and observations of star cluster disruption. The three main phases and corresponding typical timescales of cluster disruption are: I) Infant Mortality (∼ 107 yr), II) Stellar Evolution (∼ 108 yr) and III) Tidal relaxation (∼ 109 yr). During all three phases there are additional tidal external perturbations from the host galaxy. In this review we focus on the physics and observations of Phase I and on population studies of Phases II & III and external perturbations (concentrating on cluster-GMC interactions). Particular attention is given to the successes and short-comings of the Lamers cluster disruption law, which has recently been shown to stand on a firm physical footing.

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 0.080 seconds