Fig. D.1.
Mass-weighted mean molecular gas density vs. χ2 for LARS 3 and 8. The (mass-weighted) mean density (log n) of the emitting gas could be derived using a novel radiative transfer approach. The models (Puschnig et al., in prep.) were minimized against observed line luminosities of CO(1–0), CO(2–1), HCN(1–0), and HCO+(1–0) for LARS 3 and additional CO(3–2) for LARS 8.
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