APEX and NOEMA observations of H2S in nearby luminous galaxies and the ULIRG Mrk 231 - A possible relation between dense gas properties and molecular outflows

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Fig. 5.

Same plot as Fig. 4 but for the luminosities of HCN 1–0. The values for the molecular mass of the outflow, M_outflow, are from Fluetsch et al. (2019). The L_HCN1−0 values are from the references in Table 6. AGN-powered outflows are indicated with the red ‘x’ symbol.

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