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Dynamical Evolution of Star Clusters - Confrontation of Theory and Observations

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Description

This volume reviews progress in the study of 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.
Release date NZ
June 30th, 1996
Audiences
  • Postgraduate, Research & Scholarly
  • Professional & Vocational
  • Undergraduate
Contributors
  • Edited by Junichiro Makino
  • Edited by Piet Hut
Illustrations
XVIII, 406 p.
Pages
406
Dimensions
155x235x23
ISBN-13
9780792340690
Product ID
2837828

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