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Fig. 8

image

Exploration of models with X-ray heating only (no dust and no CR). The predicted line fluxes (model/observation) are plotted against each model parameter with from top to bottom, the dust mass and H0 mass (log M), minimum temperature (K) and maximum density (log  cm-3) in the radiation-bounded sector, and the X-ray luminosity (log L). Each point represents a model, and the symbol size is inversely proportional to the residuals between model predictions and observations for [C ii], [O i], and [Si ii]. The light gray zone corresponds to the observed values and their associated error bar. The dark gray zone corresponds to the best models.

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