Open Access
Table A.1.
Parameter selection for the photoionisation and shock models.
H II Regions | |
---|---|
Model reference | Pérez-Montero (2014) |
log(U) | (-4.00, -1.50) in steps of 0.25 |
12+log(O/H) | (7.1, 9.1) in steps of 0.1 |
Constraints | C tied to O |
log(N/O) | (-0.825, -0.625) in steps of 0.125 |
Planetary Nebulae | |
Model reference | Delgado-Inglada et al. (2014) |
Central star L/(102 L⊙) | (2, 10, 30, 56, 100, 178) |
SED | T.Rauch (TR) models (Rauch 2003) |
Central star Teff/(103 K) | (50 − 180) in steps of 25 |
Dust depletion | Yes |
Density [cm−3] | (30, 100, 300) |
Radius [1017 cm] | (1, 3) |
12 + log(O/H) | 8.34 |
Model set | matter bounded models (M40) |
Shock Regions | |
Model reference | Allen et al. (2008) |
Abundances | LMC (Russell & Dopita 1992) |
Magnetic field [μG] | (0.0001, 0.5, 1, 2, 3.23, 4, 5, 10) |
Shock velocities [km s−1] | (10 − 100) in steps of 25 |
Pre-shock density [cm−3] | 1 |
Model set | Shock w/o precursor |
DIG | |
Model reference | Flores-Fajardo et al. (2011) |
log(U) | (-4.0 − -3.0) in steps of 0.1 |
ϕOB | (3.50 − 5.00) in steps of 0.25 |
log(N/O) | -1.1, -0.9, -0.8, -0.7, -0.6 |
12 + log(O/H) | (7.7 − 9.3) in steps of 0.1 |
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