MWSC 5122
Summary
MWSC 5122 is a poorly populated, very loose object of very low C3 quality. It is located at a relatively close 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) | 175.98 | -28.798 | – | -9.23 | 6.21 | – |
| Bica et al. (2019) | 175.976 | -28.797 | – | – | – | – |
| UCC | 175.979 | -28.747 | 0.665 | -14.208 | -1.087 | 18.659 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.167, distance=1947, log_age=9.5 |
Search coordinates in Bayestar19