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Table 1:

Clustering measures obtained for artificial star clusters.
Cluster type      
or name $\bar{s}$ $\bar{m}$ Q
2D Uniform  
2D0 ( $N \propto r^0$) $.88\pm.03$ $.65 \pm0.02$ $.74 \pm.02 $
Radially clustered  
3D-2 ( $n \propto r^{-2}$) $.60\pm.03$ $.55 \pm.02 $ $.93 \pm .03$
3D-1 ( $n \propto r^{-1}$) $.73\pm.03$ $.61 \pm.02 $ $.84 \pm .02$
3D0 ( $n \propto r^0$) $.80\pm.02$ $.63\pm.02 $ $.79 \pm .02$
Radially anticlustered  
3D05 ( $n \propto r^{0.5}$) $.82\pm.03$ $.63\pm.02 $ $.77 \pm.02$
3D1 ( $n \propto r^{1.0}$) $.83\pm.03$ $.63\pm.02 $ $.76 \pm.02$
3D15 ( $n \propto r^{1.5}$) $.85\pm.03$ $.64\pm.02 $ $.75 \pm.02$
Fractally clustered  
F2.5 (D = 2.5) $.74\pm.09$ $.54 \pm.05$ $.73\pm.06$
F2.0 (D = 2.0) $.67\pm.13$ $.41 \pm.04$ $.61\pm.08$
F1.5 (D = 1.5) $.62\pm.18$ $.27 \pm.07$ $.45\pm.09$

Source LaTeX | All tables | In the text

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