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OverviewThis volume reviews progress in the study of the dynamics of star clusters. It focuses on the progress of both the observation and the theoretical modelling of star clusters. Results from the refurbished Hubble Space Telescope (HST) include the mass function down to the hydrogen burning limits, white dwarf sequence, and central density profiles of ""post-collapse"" clusters by star counts. On the theoretical side, this symposium saw the first direct evidence of gravothermal oscillation through N-body simulation, which was made possible by GRAPE-4, the dedicated special-purpose computer for N-body simulation. Numerical techniques to combine stellar evolution and dynamical evolution of the cluster were presented. The book will be of primary interest to astrophysicists. Full Product DetailsAuthor: Piet Hut , Junichiro MakinoPublisher: Springer Imprint: Springer Edition: 1996 ed. Volume: 174 Dimensions: Width: 16.00cm , Height: 2.20cm , Length: 24.00cm Weight: 1.320kg ISBN: 9780792340706ISBN 10: 0792340701 Pages: 406 Publication Date: 30 June 1996 Audience: College/higher education , Professional and scholarly , Undergraduate , Postgraduate, Research & Scholarly Format: Paperback Publisher's Status: Active Availability: In Print ![]() This item will be ordered in for you from one of our suppliers. Upon receipt, we will promptly dispatch it out to you. For in store availability, please contact us. Table of ContentsReviewsAuthor InformationTab Content 6Author Website:Countries AvailableAll regions |