Dynamical Evolution of Star Clusters - Confrontation of Theory and Observations
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"Dynamical Evolution of Star Clusters - Confrontation of Theory and Observations" by International Astronomical Union. Symposium, International Astronomical Union is a mathematics book and learning resource focused on Deep Sky & Solar System. Best for teachers, students, and readers looking for stronger mathematical understanding.
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.
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"Dynamical Evolution of Star Clusters - Confrontation of Theory and Observations" by International Astronomical Union. Symposium, International Astronomical Union is a mathematics book and learning resource focused on Deep Sky & Solar System. Best for teachers, students, and readers looking for stronger mathematical understanding.
Topic: Deep Sky & Solar System
Author: International Astronomical Union. Symposium, International Astronomical Union
Who this is for:
- Teachers and classroom instructors
- Students building subject mastery
- Readers looking for practical learning support
Why this book matters: It stands out as a practical math resource that helps explain concepts, strengthen problem-solving, and support classroom or independent learning.
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.
| Author | International Astronomical Union. Symposium, International Astronomical Union |
| Publisher | Springer |
| Published | 1996-06-30 |
| ISBN-13 | 9780792340706 |
| Binding | Paperback |
| Pages | 436 |
| Language | English |
| Subjects | Mathematics |
| Topic | Deep Sky & Solar System |
| Series | International Astronomical Union Symposia |
Format: Paperback
Length: 436 pages
Language: English
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