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{ "item_title" : "Dynamical Evolution of Star Clusters - Confrontation of Theory and Observations", "item_author" : [" Piet Hut", "Junichiro Makino "], "item_description" : "This volume reviews recent progress in the study of dynamics of star clusters. The meeting focused on the enormous progress of both the observation and the theoretical modeling of star clusters. New 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 ofpost-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.", "item_img_path" : "https://covers3.booksamillion.com/covers/bam/0/79/234/070/0792340701_b.jpg", "price_data" : { "retail_price" : "169.99", "online_price" : "169.99", "our_price" : "169.99", "club_price" : "169.99", "savings_pct" : "0", "savings_amt" : "0.00", "club_savings_pct" : "0", "club_savings_amt" : "0.00", "discount_pct" : "10", "store_price" : "" } }
Dynamical Evolution of Star Clusters - Confrontation of Theory and Observations|Piet Hut

Dynamical Evolution of Star Clusters - Confrontation of Theory and Observations

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Overview

This volume reviews recent progress in the study of dynamics of star clusters. The meeting focused on the enormous progress of both the observation and the theoretical modeling of star clusters. New 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.

This item is Non-Returnable

Details

  • ISBN-13: 9780792340706
  • ISBN-10: 0792340701
  • Publisher: Springer
  • Publish Date: June 1996
  • Dimensions: 9.21 x 6.14 x 0.87 inches
  • Shipping Weight: 1.31 pounds
  • Page Count: 406

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