Dynamics of Star Clusters
Proceeding of the 113th Symposium of the International Astronomical Union, Held in Princeton, New Jersey, U.S.A, 29 May - 1 June, 1984
Herausgegeben von Goodman, Jeremy; Hut, Piet
Dynamics of Star Clusters
Proceeding of the 113th Symposium of the International Astronomical Union, Held in Princeton, New Jersey, U.S.A, 29 May - 1 June, 1984
Herausgegeben von Goodman, Jeremy; Hut, Piet
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The emphasis in these proceedings of lAD Symposium No. 113, Dynafrri-,'!s of Star Clusters. and·.~.Le. mab rPIHlon for orZ'lnizinp: thE" symposium in the spring of 1984, was the rapid increase during the preceeding year in our understanding of core collapse. The last I.A.D. Symposium to discuss the dynamics of star clusters at length was No.69, Dynamics of Stellar Systems~ held in Besan~on in 1974. For a few years afterwards, globular clusters receiveu much attention due to the discovery of X-ray bursters and the mounting evidence that X-ray sources in globular clusters were formed in…mehr
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- Produktdetails
- International Astronomical Union Symposia .113
- Verlag: Springer Netherlands / Springer, Berlin
- 1985.
- Seitenzahl: 644
- Erscheinungstermin: 30. April 1985
- Englisch
- Gewicht: 1340g
- ISBN-13: 9789027719638
- ISBN-10: 9027719632
- Artikelnr.: 27619891
- Herstellerkennzeichnung
- Libri GmbH
- Europaallee 1
- 36244 Bad Hersfeld
- 06621 890
- International Astronomical Union Symposia .113
- Verlag: Springer Netherlands / Springer, Berlin
- 1985.
- Seitenzahl: 644
- Erscheinungstermin: 30. April 1985
- Englisch
- Gewicht: 1340g
- ISBN-13: 9789027719638
- ISBN-10: 9027719632
- Artikelnr.: 27619891
- Herstellerkennzeichnung
- Libri GmbH
- Europaallee 1
- 36244 Bad Hersfeld
- 06621 890
Observed Surface Densities in Globular Clusters.
Radial Velocities and Proper Motions of Globular Cluster Stars.
Chemical Gradients in Globular Clusters.
X
Raying the Dynamics of Globular Clusters.
A High Spatial Resolution Investigation of the Core of Some Dynamically Evolved Globular Clusters.
Dynamical Modeling of M13 Proper Motions.
The Dynamics of 47 Tucanae.
A Search for Post
Collapse Cores.
Core and Tidal Radii of the Carina Dwarf Spheroidal Galaxy from UK Schmidt Telescope Plates.
A Deep Luminosity Function for 47 Tucanae.
Observed Dynamical Parameters of Star Clusters in the SMC.
Where's the CUSP? (Or CCD Photometry of Globular Cluster Cores).
Rotational Field and Velocity Dispersion in Globular Clusters: ? Cen And 47 Tuc.
BV Concentric Aperture Photometry of Globular Clusters.
An Extension of the Search for Spectroscopic Binaries in M3.
A Search for Cataclysmic Binaries in the Globular Cluster M3.
Possible Characteristics of Supernova Induced Enrichment of Globular Clusters.
Dynamical Evolution of Globular Clusters.
Precollapse Evolution of Globular Clusters.
Dynamical Evolution of Globular Clusters After Core Collapse.
May 30 Model system in the Point
Mass Approximation.
Direct Fokker
Planck Calculations.
Close Encounters.
Dynamical Evolution of Multi
Component Clusters.
Gaseous Models.
Gravothermal Oscillations.
Binary Formation and Interactions with Field Stars.
Direct N
Body Calculations.
A Unified N
Body and Statistical Treatment of Stellar Dynamics.
Direct N
Body Simulations with a Recursive Center of Mass Reduction and Regularization.
Rotation and Flattening of Globular Clusters.
Dynamical Instabilities on Spherical Stellar Systems.
Why are Stellar Systems Anisotropic?.
AStatistical Treatment of Low
N Systems.
Minimum of the Eccentricity of the Galactic Globular Cluster Orbits.
Functional Integrals in Stellar Dynamics.
Multi
Component Models for the Structure and Evolution of Spherical Stellar Systems.
The Role of Hard Binaries in Cluster Evolution.
Collisional Stellar Dynamics in General Relativity: An Overview.
3
Integral Models for Globular Clusters.
The Early Stages of Post
Collapse Cluster Evolution.
Numerical Simulations of Encounters of Hard Binaries.
Collisional Relaxation: A New Approach.
May 31 External Fields and Finite
Star
Size Effects.
Tidal Effects on Globular Clusters.
Physical Interactions Between Stars.
Monte
Carlo Calculations.
Monte Carlo Simulations Of The 2+1 Dimensional Fokker
Planck Equation: Spherical Star Clusters Containing Massive, Central Black Holes.
Can a Moderately Massive Black Hole Reverse Core Collapse?.
Two Body Capture in Large N Body Systems.
Black
Hole Remnants in Globular Clusters.
Tidal Stripping and Disruption of Globular Clusters.
Open Cluster.
The Structure and Internal Kinematics of Open Clusters.
Dynamics of Open Star Clusters.
The Dynamical Evolution of Young Open Clusters.
The Dense Stellar Cores of Giant HII Regions.
N
Body Simulations of Realistic Open Clusters.
A Proper Motion Study of the Pleiades Cluster.
June 1 The Dynamics of star Clusters: Future Prospects.
Space Telescope Observations of Globular Clusters.
What Next? Priorities in Theory and Observations.
Some Summary Remarks.
Appendix I.
Appendix II.
Appendix III.
Appendix IV.
Index of Names.
Index of Subjects.
Observed Surface Densities in Globular Clusters.
Radial Velocities and Proper Motions of Globular Cluster Stars.
Chemical Gradients in Globular Clusters.
X
Raying the Dynamics of Globular Clusters.
A High Spatial Resolution Investigation of the Core of Some Dynamically Evolved Globular Clusters.
Dynamical Modeling of M13 Proper Motions.
The Dynamics of 47 Tucanae.
A Search for Post
Collapse Cores.
Core and Tidal Radii of the Carina Dwarf Spheroidal Galaxy from UK Schmidt Telescope Plates.
A Deep Luminosity Function for 47 Tucanae.
Observed Dynamical Parameters of Star Clusters in the SMC.
Where's the CUSP? (Or CCD Photometry of Globular Cluster Cores).
Rotational Field and Velocity Dispersion in Globular Clusters: ? Cen And 47 Tuc.
BV Concentric Aperture Photometry of Globular Clusters.
An Extension of the Search for Spectroscopic Binaries in M3.
A Search for Cataclysmic Binaries in the Globular Cluster M3.
Possible Characteristics of Supernova Induced Enrichment of Globular Clusters.
Dynamical Evolution of Globular Clusters.
Precollapse Evolution of Globular Clusters.
Dynamical Evolution of Globular Clusters After Core Collapse.
May 30 Model system in the Point
Mass Approximation.
Direct Fokker
Planck Calculations.
Close Encounters.
Dynamical Evolution of Multi
Component Clusters.
Gaseous Models.
Gravothermal Oscillations.
Binary Formation and Interactions with Field Stars.
Direct N
Body Calculations.
A Unified N
Body and Statistical Treatment of Stellar Dynamics.
Direct N
Body Simulations with a Recursive Center of Mass Reduction and Regularization.
Rotation and Flattening of Globular Clusters.
Dynamical Instabilities on Spherical Stellar Systems.
Why are Stellar Systems Anisotropic?.
AStatistical Treatment of Low
N Systems.
Minimum of the Eccentricity of the Galactic Globular Cluster Orbits.
Functional Integrals in Stellar Dynamics.
Multi
Component Models for the Structure and Evolution of Spherical Stellar Systems.
The Role of Hard Binaries in Cluster Evolution.
Collisional Stellar Dynamics in General Relativity: An Overview.
3
Integral Models for Globular Clusters.
The Early Stages of Post
Collapse Cluster Evolution.
Numerical Simulations of Encounters of Hard Binaries.
Collisional Relaxation: A New Approach.
May 31 External Fields and Finite
Star
Size Effects.
Tidal Effects on Globular Clusters.
Physical Interactions Between Stars.
Monte
Carlo Calculations.
Monte Carlo Simulations Of The 2+1 Dimensional Fokker
Planck Equation: Spherical Star Clusters Containing Massive, Central Black Holes.
Can a Moderately Massive Black Hole Reverse Core Collapse?.
Two Body Capture in Large N Body Systems.
Black
Hole Remnants in Globular Clusters.
Tidal Stripping and Disruption of Globular Clusters.
Open Cluster.
The Structure and Internal Kinematics of Open Clusters.
Dynamics of Open Star Clusters.
The Dynamical Evolution of Young Open Clusters.
The Dense Stellar Cores of Giant HII Regions.
N
Body Simulations of Realistic Open Clusters.
A Proper Motion Study of the Pleiades Cluster.
June 1 The Dynamics of star Clusters: Future Prospects.
Space Telescope Observations of Globular Clusters.
What Next? Priorities in Theory and Observations.
Some Summary Remarks.
Appendix I.
Appendix II.
Appendix III.
Appendix IV.
Index of Names.
Index of Subjects.