MWSC 5323
Summary
MWSC 5323 is a poorly populated, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, well above 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) | 246.765 | -7.17 | – | 2.94 | -6.94 | – |
| Bica et al. (2019) | 246.756 | -7.165 | – | – | – | – |
| UCC | 246.788 | -7.16 | 0.216 | -3.382 | -3.945 | -13.814 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.396, distance=1925, log_age=9.375 |
Search coordinates in Bayestar19