Fig. 9.
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Model HCN(1–0) luminosities as a function of the model TIR luminosities. The upper solid line corresponds to L′HCN/LTIR = 980 (Jiménez-Donaire et al. 2019), and the dashed lines are offset by a factor of 0.5 and 2. The lower solid line corresponds to a 2.3 lower L′HCN/LTIR as found for luminous IR galaxies by García-Burillo et al. (2012).
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