Fig. 7.

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[O III]88 μm/[N II]122 μm luminosity ratio as a function of metallicity Z and hardness of the photoionizing radiation, parameterized as the temperature of an equivalent black body, T*, computed from Cloudy models assuming a gas density of n = 180 cm−3. The shaded area marks the observed line ratio and its 1-σ confidence interval. The line ratio is nearly independent of metallicity at Z ≲ 0.5 Z⊙ (see Eq. (17)), while it is strongly sensitive to the hardness of the ionizing radiation. Our observations point to a value of T* = 21 000–32 000 K.
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