diff --git a/doc/RTD/source/SubgridModels/EAGLE/index.rst b/doc/RTD/source/SubgridModels/EAGLE/index.rst index 2bb720324787ed165995bc5c53887ec4a4e16c52..95f3385294b3c83834803b30af8daae6eec35070 100644 --- a/doc/RTD/source/SubgridModels/EAGLE/index.rst +++ b/doc/RTD/source/SubgridModels/EAGLE/index.rst @@ -651,6 +651,9 @@ whilst for the more recent runs we use: Supernova feedback: Dalla Vecchia+2012 & Schaye+2015 ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ +Supernova and enrichment parameters in the EAGLE-Ref model +~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ + .. code:: YAML # EAGLE stellar enrichment and feedback model @@ -675,9 +678,8 @@ Supernova feedback: Dalla Vecchia+2012 & Schaye+2015 SNII_energy_fraction_n_0_H_p_cm3: 1.4588 # Pivot point for the birth density dependance of the SNII energy fraction in cm^-3. SNII_energy_fraction_n_Z: 0.8686 # Power-law for the metallicity dependance of the SNII energy fraction. SNII_energy_fraction_n_n: 0.8686 # Power-law for the birth density dependance of the SNII energy fraction. - SNIa_DTD: PowerLaw # Functional form of the SNIa delay time distribution Two choices: 'PowerLaw' or 'Exponential'. + SNIa_DTD: Exponential # Functional form of the SNIa delay time distribution Two choices: 'PowerLaw' or 'Exponential'. SNIa_DTD_delay_Gyr: 0.04 # Stellar age after which SNIa start in Gyr (40 Myr corresponds to stars ~ 8 Msun). - SNIa_DTD_power_law_norm_p_Msun: 0.0012 # Normalization of the SNIa delay time distribution in the power-law DTD case (in Msun^-1). SNIa_DTD_exp_norm_p_Msun: 0.002 # Normalization of the SNIa delay time distribution in the exponential DTD case (in Msun^-1). SNIa_DTD_exp_timescale_Gyr: 2.0 # Time-scale of the SNIa delay time distribution in the exponential DTD case (in Gyr). SNIa_energy_erg: 1.0e51 # Energy of one SNIa explosion in ergs. @@ -690,7 +692,7 @@ Supernova feedback: Dalla Vecchia+2012 & Schaye+2015 SNII_yield_factor_Nitrogen: 1.0 # (Optional) Correction factor to apply to the Nitrogen yield from the SNII channel. SNII_yield_factor_Oxygen: 1.0 # (Optional) Correction factor to apply to the Oxygen yield from the SNII channel. SNII_yield_factor_Neon: 1.0 # (Optional) Correction factor to apply to the Neon yield from the SNII channel. - SNII_yield_factor_Magnesium: 4.0 # (Optional) Correction factor to apply to the Magnesium yield from the SNII channel. + SNII_yield_factor_Magnesium: 2.0 # (Optional) Correction factor to apply to the Magnesium yield from the SNII channel. SNII_yield_factor_Silicon: 1.0 # (Optional) Correction factor to apply to the Silicon yield from the SNII channel. SNII_yield_factor_Iron: 0.5 # (Optional) Correction factor to apply to the Iron yield from the SNII channel. @@ -699,9 +701,7 @@ different from the value (:math:`0.67`) reported in table 3 of `Schaye (2015) <http://adsabs.harvard.edu/abs/2015MNRAS.446..521S>`_ , as a factor of :math:`h^{-2} = 0.6777^{-2} = 2.1773` is missing in the paper. -The Magnesium yields from SNII have also been doubled since the -original EAGLE simulations were run and the minimal mass for SNII stars has -been raised to 8 solar masses (from 6). +The minimal mass for SNII stars has been raised to 8 solar masses (from 6).