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"Relativistic Binaries in Globular Clusters"
Matthew J. Benacquista and Jonathan M. B. Downing
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Abstract
1
Introduction
2
Globular Clusters
2.1
Stellar populations in globular clusters
2.2
The structure of globular clusters
2.3
The dynamical evolution of globular clusters
3
Observations
3.1
Cataclysmic variables
3.2
Low-mass X-ray binaries
3.3
Millisecond pulsars
3.4
Black holes
3.5
Extragalactic globular clusters
4
Relativistic Binaries
4.1
Binary evolution
4.2
Mass transfer
4.3
Globular cluster processes
5
Dynamical Evolution
5.1
Star cluster simulation methods
5.2
Results from models of globular clusters
5.3
Intermediate-mass black holes
6
Prospects of Gravitational Radiation
7
Summary
Acknowledgements
References
Updates
Figures
Tables
Figure 7:
X-ray luminosity functions for several individual galaxies. Each can be fit will with a single power law. Image reproduced by permission from Kim & Fabbiano
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, copyright by IOP.