Milone et al. 2017 classified some of these systems as “metal-complex” since pseudo two-color diagrams of them are more complicated than the typical chromosome-like shape. These systems are characterized by an anticorrelation between sodium and oxygen abundances. The high nitrogen content of the galaxy GN-z11 supports the hypothesis that some of these systems, classified as Type II by Pieter Oosterhoff, are remnants of the nuclei of disrupted (*) dwarf galaxies. A prototypical one of these systems, 47 Tucanae, (-5[1])contains (10[1])an intermediate-mass black hole as well as many millisecond pulsars, RR Lyrae stars, and blue stragglers. (10[1])The brightest of these long-lived, gravitationally bound systems of Population II stars (10[1]-5[1])is Omega Centauri. For 10 points, what spherical groups of stars (10[2])are larger (10[1])than their (10[1])“open” counterparts? (10[2])■END■ (10[3])