Table 1
List of the models described in this work.
| Models | Infall type | τd | Threshold | Radial inflow | |
|
|
|||||
| S1I | 1 infall | 1.033 R (kpc) −1.27 Gyr | no | / | |
| S1N | 1 infall | 4 Gyr | no | / | |
| S1IT4 | 1 infall | 1.033 R (kpc) −1.27 Gyr | 4 M⊙ pc-2 | / | |
| S1IT7 | 1 infall | 1.033 R (kpc) −1.27 Gyr | 7 M⊙ pc-2 | / | |
| S2IT | 2 infall | 1.033 R (kpc) −1.27 Gyr | 7 M⊙ pc-2 (thin disk phase) | / | |
| 4 M⊙ pc-2 (halo thick disk phase) | |||||
| R1I1 | 1 infall | 1.033 R (kpc) −1.27 Gyr | no | −1 km s-1 | |
| R1N1 | 1 infall | 4 Gyr | no | −1 km s-1 | |
| R1IL | 1 infall | 1.033 R (kpc) −1.27 Gyr | no | linear inflow pattern | |
| R1IT01 | 1 infall | 1.033 R (kpc) −1.27 Gyr | 4 M⊙ pc-2 | −0.1 km s-1 | |
| R1IT05 | 1 infall | 1.033 R (kpc) −1.27 Gyr | 4 M⊙ pc-2 | −0.5 km s-1 | |
| R2ITV | 2 infall | 1.033 R (kpc) −1.27 Gyr | 7 M⊙ pc-2 (thin disk phase) | variable inflow pattern | |
| 4 M⊙ pc-2 (halo thick disk phase) | |||||
Notes. The first letter in the model names is S if that model is a “static” one, otherwise R if we show a model with radial flow of gas. The following number (1 or 2) is related to the number of infall, the letter I is for the case of inside-out formation and N for a constant formation timescale along the disk. When we consider a threshold in the star formation we label that with a T. The last letter in the names of models with radial flow is related to the speed of the radial flow.
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