OC 0247
Summary
OC 0247 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 was recently reported in the literature.
This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry.
Warning: contains less than 25 stars with P>0.5 estimated.
Warning: the low UTI value and no obvious signs of duplication (C_dup=0.84) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Hao et al. (2022) | 34.628 | 56.807 | 0.387 | -0.637 | -1.187 | – |
| UCC | 34.612 | 56.847 | 0.383 | -0.618 | -1.184 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hao et al. (2022) | AG=0.46, age=7.4, Z=0.028 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWWDL 232 | 16.0 | 34.4 | 56.66 | 0.39 | -0.68 | -1.2 | – | 0.19 |
| NGC 869 | 16.0 | 34.75 | 57.14 | 0.4 | -0.66 | -1.13 | -50.34 | 1.0 |