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Fig. 11

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Ratio of the CO and [O I] luminosities as a function of preshock density for UV irradiated C–shock models and observations of Gy 3-7 cores and IM YSOs from Matuszak et al. (2015; light blue box). All models correspond to UV fields parameterized by G0 of 10 (in blue) and 0.1 (in orange). Solid lines connect models with shock velocities vs of 20 km s−1, and dashed lines – the models with vs of 10 km s−1.

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