Predicting HCN, HCO, multi-transition CO, and dust emission of star-forming galaxies - From local spiral and ultraluminous infrared galaxies to high-z star-forming and submillimeter galaxies

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Fig. 1

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Ratio between the cooling by CO, H₂, and H₂O (Neufeld & Kaufman 1993; Neufeld et al. 1995) and the cooling function proposed by Goldsmith (2001) for light (plus signs) and massive (triangles) self-gravitating molecular clouds. The symbol sizes are proportional to the scaling factor ζ (see text).

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