UBC 606
Summary
UBC 606 is a sparse, very loose object of high C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It is rarely studied in the literature.
This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry.
Warning: contains less than 25 stars with P>0.5 estimated.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2021) | 37.463 | 57.371 | 0.407 | -0.287 | -1.154 | – |
| Almeida et al. (2025) | 37.463 | 57.371 | – | – | – | – |
| UCC | 37.623 | 57.273 | 0.411 | -0.278 | -1.134 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2021) | Av=2.168, Dist=2463, logage=7.0, [Fe/H]=-0.127 |
| Almeida et al. (2025) | AV=2.168, Dist=2463, logAge=7.0, MassRk=220.1 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| UBC 192 | 40.0 | 37.05 | 57.16 | 0.4 | -0.43 | -1.15 | -27.22 | 0.54 |
| Collinder 28 | 24.0 | 38.34 | 57.55 | 0.42 | -0.28 | -1.1 | -37.49 | 0.96 |