Update all the EAGLE examples to use the new SNII feedback mode options

examples/EAGLE_ICs/EAGLE_100/eagle_100.yml

@@ -176,6 +176,7 @@ EAGLEFeedback:
   IMF_max_mass_Msun:                  100.0             # Maximal stellar mass considered for the Chabrier IMF in solar masses.
   SNII_min_mass_Msun:                   8.0             # Minimal mass considered for SNII stars in solar masses.
   SNII_max_mass_Msun:                 100.0             # Maximal mass considered for SNII stars in solar masses.
+  SNII_feedback_model:                  MinimumDistance # Feedback modes: Random, Isotropic, MinimumDistance, MinimumDensity
   SNII_sampled_delay:                   1               # Sample the SNII lifetimes to do feedback.
   SNII_delta_T_K:                       3.16228e7       # Change in temperature to apply to the gas particle in a SNII thermal feedback event in Kelvin.
   SNII_energy_erg:                      1.0e51          # Energy of one SNII explosion in ergs.

examples/EAGLE_ICs/EAGLE_12/eagle_12.yml

@@ -175,6 +175,7 @@ EAGLEFeedback:
   IMF_max_mass_Msun:                  100.0             # Maximal stellar mass considered for the Chabrier IMF in solar masses.
   SNII_min_mass_Msun:                   8.0             # Minimal mass considered for SNII stars in solar masses.
   SNII_max_mass_Msun:                 100.0             # Maximal mass considered for SNII stars in solar masses.
+  SNII_feedback_model:                  MinimumDistance # Feedback modes: Random, Isotropic, MinimumDistance, MinimumDensity
   SNII_sampled_delay:                   1               # Sample the SNII lifetimes to do feedback.
   SNII_delta_T_K:                       3.16228e7       # Change in temperature to apply to the gas particle in a SNII thermal feedback event in Kelvin.
   SNII_energy_erg:                      1.0e51          # Energy of one SNII explosion in ergs.

examples/EAGLE_ICs/EAGLE_25/eagle_25.yml

@@ -175,6 +175,7 @@ EAGLEFeedback:
   IMF_max_mass_Msun:                  100.0             # Maximal stellar mass considered for the Chabrier IMF in solar masses.
   SNII_min_mass_Msun:                   8.0             # Minimal mass considered for SNII stars in solar masses.
   SNII_max_mass_Msun:                 100.0             # Maximal mass considered for SNII stars in solar masses.
+  SNII_feedback_model:                  MinimumDistance # Feedback modes: Random, Isotropic, MinimumDistance, MinimumDensity
   SNII_sampled_delay:                   1               # Sample the SNII lifetimes to do feedback.
   SNII_delta_T_K:                       3.16228e7       # Change in temperature to apply to the gas particle in a SNII thermal feedback event in Kelvin.
   SNII_energy_erg:                      1.0e51          # Energy of one SNII explosion in ergs.

examples/EAGLE_ICs/EAGLE_50/eagle_50.yml

@@ -173,6 +173,7 @@ EAGLEFeedback:
   IMF_max_mass_Msun:                  100.0             # Maximal stellar mass considered for the Chabrier IMF in solar masses.
   SNII_min_mass_Msun:                   8.0             # Minimal mass considered for SNII stars in solar masses.
   SNII_max_mass_Msun:                 100.0             # Maximal mass considered for SNII stars in solar masses.
+  SNII_feedback_model:                  MinimumDistance # Feedback modes: Random, Isotropic, MinimumDistance, MinimumDensity
   SNII_sampled_delay:                   1               # Sample the SNII lifetimes to do feedback.
   SNII_delta_T_K:                       3.16228e7       # Change in temperature to apply to the gas particle in a SNII thermal feedback event in Kelvin.
   SNII_energy_erg:                      1.0e51          # Energy of one SNII explosion in ergs.

examples/EAGLE_ICs/EAGLE_50_low_res/eagle_50.yml

@@ -172,6 +172,7 @@ EAGLEFeedback:
   IMF_max_mass_Msun:                  100.0             # Maximal stellar mass considered for the Chabrier IMF in solar masses.
   SNII_min_mass_Msun:                   8.0             # Minimal mass considered for SNII stars in solar masses.
   SNII_max_mass_Msun:                 100.0             # Maximal mass considered for SNII stars in solar masses.
+  SNII_feedback_model:                  MinimumDistance # Feedback modes: Random, Isotropic, MinimumDistance, MinimumDensity
   SNII_sampled_delay:                   1               # Sample the SNII lifetimes to do feedback.
   SNII_delta_T_K:                       3.16228e7       # Change in temperature to apply to the gas particle in a SNII thermal feedback event in Kelvin.
   SNII_energy_erg:                      1.0e51          # Energy of one SNII explosion in ergs.

examples/EAGLE_ICs/EAGLE_6/eagle_6.yml

@@ -175,6 +175,7 @@ EAGLEFeedback:
   IMF_max_mass_Msun:                  100.0             # Maximal stellar mass considered for the Chabrier IMF in solar masses.
   SNII_min_mass_Msun:                   8.0             # Minimal mass considered for SNII stars in solar masses.
   SNII_max_mass_Msun:                 100.0             # Maximal mass considered for SNII stars in solar masses.
+  SNII_feedback_model:                  MinimumDistance # Feedback modes: Random, Isotropic, MinimumDistance, MinimumDensity
   SNII_sampled_delay:                   1               # Sample the SNII lifetimes to do feedback.
   SNII_delta_T_K:                       3.16228e7       # Change in temperature to apply to the gas particle in a SNII thermal feedback event in Kelvin.
   SNII_energy_erg:                      1.0e51          # Energy of one SNII explosion in ergs.

examples/EAGLE_low_z/EAGLE_12/eagle_12.yml

@@ -159,6 +159,7 @@ EAGLEFeedback:
   IMF_max_mass_Msun:                  100.0             # Maximal stellar mass considered for the Chabrier IMF in solar masses.
   SNII_min_mass_Msun:                   6.0             # Minimal mass considered for SNII stars in solar masses.
   SNII_max_mass_Msun:                 100.0             # Maximal mass considered for SNII stars in solar masses.
+  SNII_feedback_model:                  Random          # Feedback modes: Random, Isotropic, MinimumDistance, MinimumDensity
   SNII_sampled_delay:                   0               # Sample the SNII lifetimes to do feedback.
   SNII_wind_delay_Gyr:                  0.03            # Time in Gyr between a star's birth and the SNII thermal feedback event when not sampling.
   SNII_delta_T_K:                       3.16228e7       # Change in temperature to apply to the gas particle in a SNII thermal feedback event in Kelvin.

examples/EAGLE_low_z/EAGLE_25/eagle_25.yml

@@ -167,6 +167,7 @@ EAGLEFeedback:
   IMF_max_mass_Msun:                  100.0             # Maximal stellar mass considered for the Chabrier IMF in solar masses.
   SNII_min_mass_Msun:                   6.0             # Minimal mass considered for SNII stars in solar masses.
   SNII_max_mass_Msun:                 100.0             # Maximal mass considered for SNII stars in solar masses.
+  SNII_feedback_model:                  Random          # Feedback modes: Random, Isotropic, MinimumDistance, MinimumDensity
   SNII_sampled_delay:                   0               # Sample the SNII lifetimes to do feedback.
   SNII_wind_delay_Gyr:                  0.03            # Time in Gyr between a star's birth and the SNII thermal feedback event when not sampling.
   SNII_delta_T_K:                       3.16228e7       # Change in temperature to apply to the gas particle in a SNII thermal feedback event in Kelvin.

examples/EAGLE_low_z/EAGLE_50/eagle_50.yml

@@ -158,6 +158,7 @@ EAGLEFeedback:
   IMF_max_mass_Msun:                  100.0             # Maximal stellar mass considered for the Chabrier IMF in solar masses.
   SNII_min_mass_Msun:                   6.0             # Minimal mass considered for SNII stars in solar masses.
   SNII_max_mass_Msun:                 100.0             # Maximal mass considered for SNII stars in solar masses.
+  SNII_feedback_model:                  Random          # Feedback modes: Random, Isotropic, MinimumDistance, MinimumDensity
   SNII_sampled_delay:                   0               # Sample the SNII lifetimes to do feedback.
   SNII_wind_delay_Gyr:                  0.03            # Time in Gyr between a star's birth and the SNII thermal feedback event when not sampling.
   SNII_delta_T_K:                       3.16228e7       # Change in temperature to apply to the gas particle in a SNII thermal feedback event in Kelvin.

examples/EAGLE_low_z/EAGLE_6/eagle_6.yml

@@ -170,6 +170,7 @@ EAGLEFeedback:
   IMF_max_mass_Msun:                  100.0             # Maximal stellar mass considered for the Chabrier IMF in solar masses.
   SNII_min_mass_Msun:                   6.0             # Minimal mass considered for SNII stars in solar masses.
   SNII_max_mass_Msun:                 100.0             # Maximal mass considered for SNII stars in solar masses.
+  SNII_feedback_model:                  Random          # Feedback modes: Random, Isotropic, MinimumDistance, MinimumDensity
   SNII_sampled_delay:                   0               # Sample the SNII lifetimes to do feedback.
   SNII_wind_delay_Gyr:                  0.03            # Time in Gyr between a star's birth and the SNII thermal feedback event when not sampling.
   SNII_delta_T_K:                       3.16228e7       # Change in temperature to apply to the gas particle in a SNII thermal feedback event in Kelvin.

examples/IsolatedGalaxy/IsolatedGalaxy_feedback/isolated_galaxy.yml

@@ -149,6 +149,7 @@ EAGLEFeedback:
   IMF_max_mass_Msun:                  100.0             # Maximal stellar mass considered for the Chabrier IMF in solar masses.
   SNII_min_mass_Msun:                   8.0             # Minimal mass considered for SNII stars in solar masses.
   SNII_max_mass_Msun:                 100.0             # Maximal mass considered for SNII stars in solar masses.
+  SNII_feedback_model:                  MinimumDistance # Feedback modes: Random, Isotropic, MinimumDistance, MinimumDensity
   SNII_sampled_delay:                   1               # Sample the SNII lifetimes to do feedback.
   SNII_delta_T_K:                       3.16228e7       # Change in temperature to apply to the gas particle in a SNII thermal feedback event in Kelvin.
   SNII_energy_erg:                      1.0e51          # Energy of one SNII explosion in ergs.