Formation of globular clusters with multiple stellar populations from massive gas clumps in high-z gas-rich dwarf galaxies

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Volume 622 (February 2019)

A&A, 622 (2019) A53

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Table 2

Summary of model parameters.

Model	M_dm (10⁹ M_⊙)	M_s (10⁹ M_⊙)	M_g (10⁹ M_⊙)	f_b	f_g	R_g (kpc)	Comments
M1	20.0	0.5	2.0	0.11	0.80	4.5	Standard model
M2	20.0	0.5	2.0	0.11	0.80	4.5	Strong SN feedback
M3	20.0	0.5	2.0	0.11	0.80	4.5	No SN feedback
M4	20.0	0.5	2.0	0.11	0.80	4.5	No AGB feedback
M5	20.0	0.5	1.0	0.07	0.67	4.5
M6	20.0	0.5	1.5	0.09	0.75	4.5
M7	20.0	1.5	1.0	0.11	0.40	4.5
M8	20.0	2.0	0.5	0.11	0.20	4.5
M9	20.0	0.1	0.4	0.02	0.80	4.5
M10	20.0	0.1	0.6	0.03	0.86	4.5
M11	20.0	0.1	1.0	0.05	0.91	4.5
M12	20.0	0.1	2.0	0.10	0.95	4.5
M13	20.0	0.5	2.0	0.11	0.80	11.3	LSB
M14	20.0	0.5	2.0	0.11	0.80	7.1	LSB
M15	20.0	0.5	2.0	0.11	0.80	2.3	Higher surface density
M16	2.0	0.05	0.2	0.11	0.80	1.4
M17	6.0	0.15	0.6	0.11	0.80	2.5
M18	60.0	1.5	6.0	0.11	0.80	7.8
M19	2.0	0.05	0.2	0.11	0.80	0.7	Higher surface density
M20	6.0	0.15	0.6	0.11	0.80	1.2	Higherpace1mm surface density
M21	60.0	1.5	3.0	0.07	0.67	7.8
M22	60.0	1.5	1.5	0.05	0.50	7.8
M23	20.0	0.5	2.0	0.11	0.80	4.5	T_g = 10³ K
M24	20.0	0.5	2.0	0.11	0.80	4.5	T_g = 10⁴ K
M25	20.0	0.5	2.0	0.11	0.80	4.5	Q_g = 0, Q_s = 1.5
M26	20.0	0.5	2.0	0.11	0.80	4.5	Q_g = Q_s = 1.5
M27	20.0	0.5	2.0	0.11	0.80	4.5	Q_g = Q_s = 3.0
M28	20.0	0.5	2.0	0.11	0.80	4.5	ρ_{th, SG} = 1 atom cm⁻³
M29	20.0	0.5	2.0	0.11	0.80	4.5	ρ_{th, SG} = 1000 atom cm⁻³

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