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Fig. 2

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Cooling and heating rate versus depth for the main mechanisms in a typical 1D model (stellar age: 6 Myr, L* = 109 L, n = 2, U = −2, Z = 0.1 Z, LX = 107 L, TX = 106 K). The dashed vertical lines correspond to the cut values 1, 2, and 3. Acronyms: “IScclinH”: hydrogen recombination; “ISrcolH”: net free-bound cooling minus free-free heating; “PE”: photoelectric effect heating; “CR”: cosmic ray heating.

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