Table 1.
Three clumps of high spatial density (shown as yellow dots in Fig. 2).
| Clump | N | M | X | Y | Z | d |
|---|---|---|---|---|---|---|
| (pc) | (pc) | (pc) | (pc) | |||
| A | 39 | 1 | −125.4 | −57.6 | −92.7 | 166.2 |
| B | 38 | 3 | −25.0 | 52.8 | −103.1 | 118.4 |
| C | 32 | 4 | 15.6 | 26.5 | −96.2 | 101.0 |
Notes. First column is the clump name, the second the number of stars in the clump. The third column gives the corresponding name of the over-densities in Meingast et al. (2019). The following four columns give the Galactic Cartesian coordinates and the distance from the Sun of the clump centres.
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