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Table 1

Initial conditions for the grid of PDR models.

[O/H] D $\mathcal{D}$ C O Comments
0.2 13.376 5.49(−4) 7.76(−4) Galactic Center
0 3.93 2.53(−4) 4.90(−4) Sun
−0.2 1.15 1.19(−4) 3.09(−4) Solar neighb.
−0.4 0.338 5.78(−5) 1.95(−4) LMC type
−0.6 0.099 2.88(−5) 1.23(−4) SMC type
−0.8 0.029 1.48(−5) 7.77(−5) Metal poor
−1.0 0.0085 7.83(−6) 4.90(−5) Extr. metal poor

Notes. The first column corresponds to the [O/H] value, the second to the D $\mathcal{D}$ dust-to-gas ratio normalized to the value of 10−2 (see Eq. (2)), the third to the carbon abundance, and the fourth to the oxygen abundance (calculated using the best-fit of Sharda et al. 2023b,a). In the fifth column, we list the most representative objects in each case.

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