Kinetic tomography of the Galactic plane within 1.25 kiloparsecs from the Sun - The interstellar flows revealed by H I and CO line emission and 3D dust

Open Access

Fig. 13

Differences between the line-of-sight velocity derived from the H I (left) and CO (right) line emission associated with the distance channels in the 3D dust reconstruction using the HOG method, $v_{L O S}^{H O G}$ $\[v_{\mathrm{LOS}}^{\mathrm{HOG}}\]$ , and the expected LOS velocities according to the Galactic rotation model presented by Reid et al. (2019), $v_{LOS}^{R 19}$ $\[v_{\text {LOS }}^{\mathrm{R} 19}\]$ .

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