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Table 2
Parameters of our models.
Galaxy | Model | Star formation rate (SFR) [M⊙/yr] | Final stellar | Initial gas |
(t is the look-back time expressed in Gyr) | mass [M⊙] | mass [M⊙] | ||
|
||||
Sculptor | A |
![]() |
~1.5 × 106 | 2 × 107 |
0 (t < 5) | ||||
B |
![]() |
~1.5 × 106 | 2 × 107 | |
0 (t < 5) | ||||
|
||||
Fornax | C |
![]() |
~4.5 × 107 | 3 × 108 |
0 (t < 1) | ||||
D |
![]() |
~4.5 × 107 | 3 × 108 | |
|
||||
Carina | E |
![]() |
~0.5 × 106 | 13 × 106 |
Notes. The models A, B, ... are further subdivided into A1, A2, B1, B2 etc.: the X1 models have a SN Ia Mn yield ∝ (Z/Z⊙)0.65, while the X2 models have a constant SN Ia Mn yield (this subdivision is not shown in the table).
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