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Table 3
ISM model parameters.
| Parameter | Description | Values/range |
|---|---|---|
| Primary parameters with distinct values for each component (sector) | ||
| w | Component (sector) mixing weight | [0–1] |
| log U0 | Ionization parameter(a) | [−4, −3, −2, −1, 0] |
| log n0 (cm−3) | Gas density(a) | [0, 1, 2, 3, 4] |
| cut | Depth into the cloud(b) | [0 – −4] step 0.25 |
| Primary parameters with a single value for all components (sectors) | ||
| log Z | Metallicity | [−2.19, −1.889, −1.1−2.−9, −1.89, −1.19, −0.889, -−0.667, −0.491, −0.19, 0.111] |
| log Zdust | Dust-to-gas mass ratio(c) | [−0.68, 0, +0.70] |
| log LX (L⊙) | X-ray source luminosity | [−∞, −3, −2, −1] |
| log TX (K) | X-ray source temperature | [0, 5, 6, 7] |
| log L* (L⊙) | Stellar cluster luminosity | [7, 9] |
| Age (Myr) | Burst age | [1, 2, 3, 4, 5, 6, 8, 10] |
| Secondary (predicted) parameters in this study | ||
| log Q(H) (s−1) | Number of ionizing photons | |
| fesc(1 – ∞) (%) | Escape fraction of photons with energy range [1 – ∞] Ryd | |
| fesc(1–1.8) (%) | Escape fraction of photons with energy range [1–1.8]Ryd | |
| fesc(1.8–4) (%) | Escape fraction of photons with energy range [1.8–4]Ryd | |
| fesc(4–20) (%) | Escape fraction of photons with energy range [4–20] Ryd | |
| fesc(20 – ∞) (%) | Escape fraction of photons with energy range [20 – ∞] Ryd | |
| MH+ (log M⊙) | Mass of H+ | |
| MH0 (log M⊙) | Mass of H0 | |
| MH2 (log M⊙) | Mass of H2 | |
| MH2,C+ (log M⊙) | Mass of H2 traced by C+ | |
| MH2,C0 (log M⊙) | Mass of H2 traced by C0 | |
| MH2,Co (log M⊙) | Mass of H2 traced by CO | |
| Mdust (log M⊙) | Dust mass | |
| fCII,H+ | Fraction of [C ii] associated with H+ | |
| fcII,H0 | Fraction of [C ii] associated with H0 | |
| fCII,H2 | Fraction of [C ii] associated with H2 | |
Notes.(a) Calculated at the illuminated face of the cloud.(b) See definition in Sect. 4.2.(c) The range [−1, 1] corresponds to the 95% envelop (in dex) around the median relationship in Galliano et al. (2021).
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