Table 4.
Distance of the Chamaeleon subgroups using different zero-point corrections for the Gaia-DR2 parallaxes.
| Sample | Nd | Distance | |
|---|---|---|---|
| (pc) |
|||
| Stassun & Torres (2018) | No correction | ||
| Cha I (north) | 76 |
 |
 |
| Cha I (south) | 84 |
 |
 |
| Cha I | 160 |
 |
 |
| Cha II | 31 |
 |
 |
Notes. We provide for each subgroup the number of stars and the Bayesian distances derived from the largest zero-point shift reported in the literature (−0.082 ± 0.033 mas, Stassun & Torres 2018) and without any zero-point correction applied to the Gaia-DR2 parallaxes.
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