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. 1

Examples of the 3D dust, ¹²CO, and H I data combined in this paper. Top: Nucleon density derived from the 3D extinction model presented by Edenhofer et al. (2024) for three distance bins indicated in the figure. Middle: ¹²CO line emission from the Dame et al. (2001) survey for the three LOS velocity intervals indicated in the figure. Bottom: H I 21-cm line emission observations presented by HI4PI Collaboration (2016).

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