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Commit 1c19a8a4 authored by Folkert Nobels's avatar Folkert Nobels
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Updates one parameter file

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......@@ -295,15 +295,15 @@ SchayeSF:
SchmidtLawHighDensExponent: 2.0 # The high density exponent for the Kennicutt-Schmidt law
SchmidtLawHighDens_thresh_HpCM3: 1e3
Schaye2004: 1 # whether to use the metallicity dependent critical star formation of Schaye (2004) (1) or not (0).
thresh_norm_HpCM3: .1 # Critical sf normalization to use (is not a normalization when Schaye2004=0, than it is the value.
thresh_norm_HpCM3: 0.1 # Critical sf normalization to use (is not a normalization when Schaye2004=0, than it is the value.
thresh_max_norm_HpCM3: 10.0 # Maximum norm of the critical sf density
MetDep_Z0: 0.002 # Scale metallicity to use for the equation (not used for Schaye2004=0)
MetDep_SFthresh_Slope: -0.64 # Scaling of the critical density with the metallicity (not used for Schaye2004=0)
thresh_MaxPhysDensOn: 0 # Default is 0.
thresh_MaxOverDens_HpCM3: 1e5 # Density at which the SF law changes
EOS_Jeans_GammaEffective: 1.33333 # The polytropic index
EOS_Jeans_TemperatureNorm_K: 1e3 # No idea how this works
EOS_JEANS_DensityNorm_HpCM3: .1 # No idea what the value is.
EOS_Jeans_TemperatureNorm_K: 1e3 # No idea how this works
EOS_JEANS_DensityNorm_HpCM3: 0.1 # No idea what the value is.
# Structure finding options (requires velociraptor)
StructureFinding:
......
......@@ -259,6 +259,8 @@ INLINE static void star_formation_copy_properties(
/* Store the birth density in the star particle */
sp->birth_density = p->rho;
message("A star has been formed!");
}
/*
......@@ -400,7 +402,7 @@ INLINE static void starformation_init_backend(
}
/* Claculate 1 over the metallicity for speed up */
/* Claculate 1 over the metallicity */
starform->Z0_inv = 1/starform->Z0;
/* Calculate the prefactor that is always common */
......
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