Table 1
Principal characteristics of the computed passive and star-forming galaxies.
| Salpeter (1955) | Chabrier (2003) | ||||||||
| Passive galaxies | Star-forming galaxies | Passive galaxies | Star-forming galaxies | ||||||
| Range | 75% | Range | 75% | Range | 75% | Range | 75% | ||
|
|
|||||||||
| Infall timescale | τ [Gyr] | 0.07−4.8 | ≤1.8 | 0.07−7.8 | ≤6 | 0.07−4.2 | ≤2.4 | 0.07−7.8 | ≤6.6 |
| Age | [Gyr] | 1.8−13.1 | ≤9.6 | 0−4.8 | ≤2.4 | 0.6−13.1 | ≤10.2 | 0−3 | ≤1.8 |
| Wind parameter | λ | 0−1.5 | ≤0.9 | 0−5.8 | ≤2.25 | 0.6−3 | ≤2.2 | 0.6−10.2 | ≤5.3 |
| Infall mass | log (Minf [M⊙]) | 9.5−11.5 | ≤10.5 | 10.1−11.5 | ≤11.43 | 10.2−11.8 | ≤10.9 | 10.8−12.5 | ≤12.05 |
Notes. In each column we indicate the range spanned by the values related to the infall timescale τ, the ages of the computed local galaxies, the wind parameter λ, and the infall mass Minf. Moreover, the range of values at which 75% of the galaxies are found is presented. Results are also indicated for two different IMFs: a Chabrier (2003); and Salpeter (1955) IMF.
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