Fig. 7.
Absolute proper motion components |pmRA| and |pmDE| of stars in the Gaia DR2 10 pc (left panels) and 20 pc samples (right panels) are plotted in logarithmic scale. Total proper motions of 5 mas yr−1, 50 mas yr−1, and 500 mas yr−1 are indicated by solid lines. The symbols for the subsamples A and B (top row) and C and D (bottom row) are the same as in Fig. 3. Two well-measured nearby stars with the smallest proper motions are marked in the top row.
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