Open Access
Table 1.
Model summary.
| Fixed parameters | |
|---|---|
| Geometry | 1D plane-parallel |
| Radiation field | Intergalactic background continuum |
| HM05 (a) at redshift 0 | |
| Table SED “cool.sed” (d) (X-ray emission), intensity (GX(c)) set to values below | |
ISRF (b) scaled to  |
|
| CMB | |
| Cosmic ray background: H0 ionization rate of 2 × 10−16 s−1 | |
| Density law | Constant pressure set to 106.5 K cm−3 |
| Varied parameters | Values |
| X-ray radiation field intensity (GX) | [10−2, 10−1.8, 10−1.6, 10−1.4, 10−1.2, 10−1, 10−0.8, 10−0.6, 10−0.4, 10−0.2, 1, 100.2, 100.4, 100.6, 100.8 10, 101.2, 101.4, 101.6, 101.8, 102, 102.2, 102.4, 102.6, 102.8, 103] |
| Metal abundances (Z) | [0.3, 0.35, 0.4, 0.45, 0.5, 0.55, 0.6, 0.65, 0.7, 0.75, 0.8, 0.85, 0.9, 0.95, 1] Z⊙ |
| Turbulent velocity(vtur) | [0, 2, 10, 30, 50, 100] km s−1 |
Notes.
(b)
Interstellar radiation field calculated by Meudon PDR code (Le Petit et al. 2006) using the radiation field from Mathis et al. (1983).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.