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Дата изменения: Fri Oct 4 23:01:32 2013
Дата индексирования: Sun Mar 2 07:21:23 2014
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Simulation Parameters
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Model Designation
(Name)
Star Formation Law
Continuous Star Formation
Star Formation Rate
M
yr
-1
Fixed Mass
Total Stellar Mass
x10
6
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
x10
6
yr
Age of the Spectrum
x10
6
yr
Mass Interpolation
Small Mass Grid
Large Mass Grid
Isochrone on Large Grid
Full Isochrone
Selected Tracks
l
min
l
max
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
x10
19
cm
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)
x10
5
Mean Temperature
x10
4
K
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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