Table 3
Young stellar associations with their respective distances to the geometric center of the group and age from Mamajek (2016).
| Name | Distance (pc) | Age (Myr) |
|---|---|---|
| AB Doradus | 20 | 150 |
| β Pictoris | 37 | 23 |
| β Tucanae | 43 | 45 |
| Tucana Horologium | 48 | 45 |
| Columba | 50 | 42 |
| TW Hydrae | 53 | 10 |
| Carina | 65 | 45 |
| 32 Orionis | 92 | 22 |
| η Chamaeleontis | 94 | 11 |
| χ 1 For | 99 | 50 |
Notes. For β Pictoris’ distance, the value found by Bonati et al. (2019) is used. Associations above the horizontal line are considered as Near, below the line as Far. The three associations studied in closer detail in this paper are highlighted in bold.
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