MWSC 4688
Summary
MWSC 4688 is a poorly populated, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, well below the mid-plane. It is rarely studied in the literature, with no articles listed in the last 6 years.
Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) 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 |
|---|---|---|---|---|---|---|
| Kharchenko et al. (2012) | 357.975 | -86.72 | – | 3.2 | -5.0 | – |
| Bica et al. (2019) | 357.959 | -86.714 | – | – | – | – |
| UCC | 357.926 | -86.719 | 0.212 | 3.252 | -1.914 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.219, distance=1336, log_age=9.39 |
Search coordinates in Bayestar19