Simulation Parameters

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Model Designation (Name)
Star Formation Law
Continuous Star Formation Star Formation RateM yr-1		Fixed Mass Total Stellar Mass x106 M
Number of IMF Intervals
IMF Exponents
Mass Boundaries for IMF		M
Supernova Cut-Off Mass		M
Black Hole Cut-Off Mass		M
Stellar Evolution
Geneva Std. 0.001 0.004 0.008 0.020 0.040		Padova Orig. 0.0004 0.004 0.008 0.020 0.050
Geneva High 0.001 0.004 0.008 0.020 0.040		Padova AGB 0.0004 0.004 0.008 0.020 0.050
Wind Model		Evolution Empirical Theoretical Elson et al.
Time Step		x106 yr
Age of the Spectrum		x106 yr
Mass Interpolation		Small Mass Grid Large Mass Grid Isochrone on Large Grid Full Isochrone
Selected Tracks lmin lmax		All Tracks
Stellar Atmospheres
Atmosphere for the Input Spectrum		Planck Lejeune Lejeune/Schmutz Lejeune/Hillier Pauldrach/Hillier
Elemental Abundances of the Gas
Default Z = 0.05 x solar Z = 0.20 x solar Z = 0.40 x solar Z = 1.00 x solar Z = 2.00 x solar		Enter Abundances for Each Element H He C N O Ne Na Mg Al Si S Cl Ar Ca Fe Ni
Dust
Include Dust		Ignore Dust
Depletion Factors
Default		Enter Indvidual Depletion Factors H He C N O Ne Na Mg Al Si S Cl Ar Ca Fe Ni
Grain Distribution Model		MRN Grain Distribution
Evaluate Dust Temperature and IR Flux
Yes		No
ISM Geometry and Ionization Source
Spherical		Plane-Parallel
Unscaled Starburst99 Spectrum     or   Scaled Starburst99 Spectrum (Enter Parameters) Define source size by one of: Source Radius R log(Total Luminosity) erg s-1 log(Ionizing Luminosity) erg s-1 Define inner ionizing radius by one of:   Distance x1019cm Stromgren Radius Fraction log(Ionization Parameter)		Scaled Starburst99 Spectrum (Enter Parameters) Define inner ionizing radius by one of: log(Ionization Parameter) Bolometric Flux erg s-1 cm-2 Ionizing Flux erg s-1 cm-2
Density Structure
Isochoric		Isobaric
Hydrogen Density cm-3		Pressure (P/K)x105    Mean Temperaturex104K
Filling Factor
Output Files
Choose One:		Standard Standard+Monitor 4 Ions Stardard+Monitor All Ions Standard+Final Source + nu F(nu) Spectrum Standard+First Balance All
If Standard+Monitor 4 Ions, Enter Ions by Atomic Number:
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