List Of Tables

List of Tables

Table 1:
Low-mass X-ray binaries in globular clusters. Host clusters and LMXB properties.

Table 2:
Quiescent Low-mass X-ray binaries in globular clusters.

Table 3:
Short-orbital-period binary millisecond pulsars in globular clusters. Host clusters and orbital properties. See External Link

http://www.naic.edu/~pfreire/GCpsr.html for references to each pulsar.

Table 4:
Structural parameters for 47 Tuc and $ω$ Cen taken from Davies and Benz [95]. $Mtot$ is the total mass, $ρ 0$ the central density, $r c$ the core radius, $r t$ the tidal radius and $t rh$ the current estimated half-mass relaxation time.

Table 5:
The mean number of eccentric binaries per cluster ( $⟨N ⟩$ ) and the Poisson probability ( $P N$ ) that at least $N$ eccentric DWDs are present at any given time. Data taken from Willems et al. 2007 [487].

Table 6:
The cumulative number of BH–BH binaries after 3, 9, and 25 $trh$ , and also after 1 $T H$ . The first column gives the initial conditions. 10 or 50 in the first place indicates 10% or 50% primordial binaries. sol or low indicates a metallicity of z = 0.02 or z = 0.001. The number in the third place indicates $rt∕rh$ = 21, 37, 75 or 180. Each column is averaged over ten independent realizations and includes the $1σ$ uncertainty. A dash in a column indicates that the cluster did not reach that number of half-mass relaxation times within one Hubble time. Reproduced by permission from Downing et al. 2010 [111]

	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