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Fig. C.2

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Standard model, from top to bottom and from left to right: Tgas with overplotted gas temperature contours (white/black) and AV = 1, 10 (red), Tdust with overplotted temperature contours (black/white) and AV = 1, 10 (red), dust-to-gas mass ratio, average dust grain size, main cooling processes (CII fine structure lines, dust grain-gas thermal exchange, Ly α line, neutral O line cooling, CO rotational and ro-vibrational cooling, water rotational and ro-vibrational cooling, formaldehyde rotational cooling, ammonia rotational cooling, OIII line cooling), main heating processes (collisional excitation of vibrationally excited H2, chemical heating due to H2 formation on dust grains, dust grain-gas thermal exchange, heating from the superthermal photo-electrons produced by C, heating by cosmic rays, heating by the photo-electrons produced by polycyclic aromatic hydrocarbons, IR heating due to the water transitions, heating by mutual electron collisions, Coulomb heating, produced by X-rays photoionization, reaction free energy heating from exothermic reactions).

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