Open Access

Table G.1

WL-PDR features

Feature details comments Ref
model geometry plane-parallel, semi-infinite
coolant excitation non-LTE level population of [O I], [C II], [C I], LAMDA database format (1)
CO, 13CO, CH, CH+, and HCO+ using an escape probability approach
Chemistry time-dependent, returned for tfinal AccuracyGoal→ | log10(n × 10−10)|
FORTRAN: atol=1e-10*n
PrecisionGoal→ 10
FORTRAN: rtol=1e-18
MaxSteps→ 109
thermal balance solved self-consistently with the chemistry iteratively
Shielding self-shielding factors for CO (2)
heating & cooling H2 processes (pumping, line cooling, formation-and dissociation processes (3),(4),(5)
gas-grain heating/cooling (6)
photoelectric heating and recombination cooling (7)
Ly-αcooling (4)
optical Oxygen-6300 Åcooling (4)
heating by C-ionization and cosmic rays (5)
line cooling by [O I], [C II], [C I] (fine structure), CO,13CO, assuming a thermalized H2 ortho/para ratio
CH, CH+, and HCO+ (rotational)
model output AV grid
chemical abundances (cm−3)
column densities to the edge of the PDR (cm−2)
gas and dust temperature (K)
heating and cooling rates (erg s−1 cm−3)
total heating and cooling rates and sum of them (erg s−1 cm−3)
surface brightness of CO, 13CO, CH, (erg s−1 cm−2 sr−1)
CH+, HCO+, [O I], [C II], and [C I]

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