MWSC 5667
Summary
MWSC 5667 is a poorly populated, very loose object of 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) | 94.5 | -31.8 | – | -0.5 | 2.14 | – |
| Bica et al. (2019) | 94.492 | -31.802 | – | – | – | – |
| UCC | 94.523 | -31.838 | 0.254 | 0.098 | 2.315 | 111.491 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.312, distance=2290, log_age=9.015 |
Search coordinates in Bayestar19