Fig. 6
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HI absorption analysis for RRL clump 1. Upper panel: HI absorption lines of RRL clump 1. Lower panel: kinematic distance estimates for sources at the Galactic longitude of RRL clump 1, which has an LSR velocity of 54 km s−1: 3.5 kpc (near) and 9.9 kpc (far). The dashed blue line marks the LSR velocity of the source, and the dotted black line the tangent point velocity.
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