OutputDir      ./                       % Output directory
OutputFile     disktest.dat             % Filename of generated initial conditions


CC             9.0	  % halo concentration
V200         160.0	  % circular velocity v_200 (in km/sec)
LAMBDA         0.033      % spin parameter          
MD             0.041      % disk mass fraction      
MB             0.01367    % bulge mass fraction     

MBH            0.0000     % black hole mass fraction. If zero, no black
                          % hole is generated, otherwise one at the centre
                          % is added.
 

JD             0.041	  % disk spin fraction, typically chosen equal to MD

GasFraction    0.1        % relative content of gas in the disk, the rest is stars
DiskHeight     0.2        % thickness of stellar disk in units of radial scale length 
BulgeSize      0.2        % bulge scale length in units of disk scale length 

N_HALO         30000      % desired number of particles in dark halo 
N_DISK         20000      % desired number of collisionless particles in disk 
N_GAS          20000      % number of gas particles in disk 
N_BULGE        10000      % number of bulge particles 

HI_GasMassFraction     0.0	% mass of extended, flat HI disk in terms of the total gas mass
HI_GasDiskScaleLength  6	% scale length of extended gas disk in terms of scale length of the disk 
MaxGasDiskHeight       1.0	% to prevent too big flaring of isothermal outer gas disk


RadialDispersionFactor 1.0      % applies to stellar disk: Gives the radial
                                % dispersion in units of the z-dispersion


MaxSfrTimescale     1.5         % Gas consumption timescale (multi-phase model)
FactorSN            0.1         % beta, mass fraction of massive stars (multi-phase model)
FactorEVP           1000        % A_0, evaporation parameter (multi-phase model)
TempSupernova       1e+08       % T_SN, effective "supernova temperature",sets feedback energy (multi-phase model)
TempClouds          1000        % temperature of cold clouds (multi-phase model)

FactorForSofterEQS  1.0         % Can be used to make the equation of state
                                % softer. For 1.0, the multiphase model is
				% used, while for 0.0 isothermal at 10^4 K is
				% assumed. Intermediate values interpolate
                                % linearly between the two pressures.