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. 8

Same as Fig. 7, but for high morphological correlation between H I and 3D dust. This example corresponds to the highest V_d in the comparison between the H I line emission and the 3D dust density presented in the left panel of Fig. 5.

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