Fig. 5.
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Measured radial velocities of the studied objects with their slit numbers (see Tables 5, 6) as a function of the galactocentric radius (Table 2). Large red numbers indicate emission-line objects. Small red numbers indicate absorption-line objects younger than 100 Myr. Black numbers indicate absorption-line objects older than 100 Myr. Dashed red line shows disk rotation.
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