Fig. 11
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Stellar density distribution in the Galactic plane for the studied sample. The map shows the number of stars per 30 × 30 pc bin on a logarithmic scale. The highest statistical significance is concentrated in the solar neighborhood (R ≈ 8.5 kpc, Z ≈ 0 kpc). Isolated pixels at larger heliocentric distances (low Z) represent low-count bins (N < 10).
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