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Population of Galactic globular clusters, figures



FIGURE. 6.—The distributions of halo clusters projected onto the XY [(a) and (c)] and YZ [(b) and (d)] planes for old-halo clusters with (B-R)/(B+V+R)&bolrov;0.85 [(a) and (b)] and young-halo clusters [(c) and (d)]. The open and filled circles in (c) and (d) show clusters with (B-R)/(B+V+R)&menrov;0.32 and (B-R)/(B+V+R)>0.32, respectively. Other notation is the same as in Fig. 2..
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