Table 1. Open in new tab Relevant...

n_thresh	T_c	P₀	P_kin	t_wind	θ	f_fb,therm	f_fb,kin	f_fb,local	f_ev	f_*	N_*	\|$M_{\ast , \rm SN}$\|
0.01	300	2 × 10⁴	0.05	15 – \|$t_{\rm dyn, c\, [Myr]}$\|	30	0.2	0.26	0.02	0.1	0.02	4	120

n_thresh	T_c	P₀	P_kin	t_wind	θ	f_fb,therm	f_fb,kin	f_fb,local	f_ev	f_*	N_*	\|$M_{\ast , \rm SN}$\|
0.01	300	2 × 10⁴	0.05	15 – \|$t_{\rm dyn, c\, [Myr]}$\|	30	0.2	0.26	0.02	0.1	0.02	4	120

Table 1.

Relevant parameters of the sub-resolution model.

n_thresh	T_c	P₀	P_kin	t_wind	θ	f_fb,therm	f_fb,kin	f_fb,local	f_ev	f_*	N_*	\|$M_{\ast , \rm SN}$\|
(cm⁻³)	(K)	(k_B K cm⁻³)		(Myr)	(°)							(M_⊙)
0.01	300	2 × 10⁴	0.05	15 – \|$t_{\rm dyn, c\, [Myr]}$\|	30	0.2	0.26	0.02	0.1	0.02	4	120

n_thresh	T_c	P₀	P_kin	t_wind	θ	f_fb,therm	f_fb,kin	f_fb,local	f_ev	f_*	N_*	\|$M_{\ast , \rm SN}$\|
(cm⁻³)	(K)	(k_B K cm⁻³)		(Myr)	(°)							(M_⊙)
0.01	300	2 × 10⁴	0.05	15 – \|$t_{\rm dyn, c\, [Myr]}$\|	30	0.2	0.26	0.02	0.1	0.02	4	120

Note. Column 1: number density threshold for multiphase particles. Column 2: temperature of the cold phase. Column 3: pressure at which the molecular fraction is f_mol = 0.5. Column 4: gas particle’s probability of becoming a wind particle. Column 5: maximum lifetime of a wind particle. Columns 6: half-opening angle of the cone for thermal feedback, in degrees. Columns 7 and 8: thermal and kinetic SN feedback energy efficiencies, respectively. Column 9: fraction of SN energy directly injected into the hot phase of the ISM. Column 10: evaporation fraction. Column 11: star formation efficiency, as a fraction of the molecular gas. Column 12: number of stellar generations, i.e. number of star particles generated by each gas particle. Column 13: average stellar masses of stars formed per each SN II.

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