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Fig. 10
Number of stars in the GUMS model for three different directions: l = 25° (left), l = 95° (middle) and l = 175° (right) in regions of angular size of Δl = ± 5° and Δb = ± 5°. The top row corresponds to super-giant (dotted lines) and giant (solid) stars, and the bottom row to sub-giant (dotted) and dwarf stars (solid).
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