Table 4.
Fraction of SySt formed through each of the defined channels in this work.
| Galaxy | Z | I | II RGBs | II RGBu | II AGBs | II AGBu | III |
|---|---|---|---|---|---|---|---|
| ×10−4 | (±0.4%) | (±1%) | (±8%) | (±0.4%) | (±2%) | (±9%) | |
| Milky Way | 140 | 0.8 | 5.7 | 9.3 | 3.2 | 2.6 | 78.5 |
| LMC | 40 | 0.6 | 6.5 | 9.6 | 3.0 | 2.7 | 77.6 |
| SMC | 10 | 0.5 | 7.3 | 9.5 | 3.2 | 3.1 | 76.5 |
| NGC 205 | 20 | 0.5 | 6.9 | 9.7 | 3.1 | 2.9 | 76.9 |
| IC 10 | 5 | 0.4 | 7.6 | 9.3 | 3.3 | 3.1 | 76.2 |
| NGC 6822 | 10 | 0.4 | 7.3 | 9.5 | 3.2 | 3.1 | 76.5 |
| NGC 185 | 5 | 0.4 | 7.7 | 9.2 | 3.3 | 3.1 | 76.4 |
| IC 1613 | 5 | 0.4 | 7.6 | 9.3 | 3.3 | 3.1 | 76.3 |
| NGC 147 | 10 | 0.4 | 7.3 | 9.5 | 3.2 | 3.1 | 76.5 |
| WLM | 5 | 0.4 | 7.6 | 9.4 | 3.3 | 3.1 | 76.2 |
| Sagittarius | 60 | 0.6 | 6.2 | 9.7 | 3.0 | 2.7 | 77.7 |
| Fornax | 10 | 0.5 | 7.3 | 9.5 | 3.2 | 3.2 | 76.5 |
Notes. Values are in percentage. The column Z expresses the PARSEC metallicity, for the stellar tracks, used for each galaxy. The letters ‘u’ and ‘s’ on the columns displaying the subchannels of channel II stand for unstable and stable, respectively. Only galaxies with nonzero derived SySt population are displayed. Uncertainties are asymmetrical, an approximation is given between parenthesis.
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