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. 14

Histograms of the physical quantities derived from the HOG analysis. Top left: Effective energy density, n_eff, that is assigned to each gas tracer, as defined in Eq. (3). Top right: Kinetic energy density, E_k, calculated with Eq. (5). Bottom left: Radial momentum, p, calculated with Eq. (7). Bottom right: Mass flow rate, $\dot{M}$ $\[\dot{M}\]$ , calculated with Eq. (8).

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