MWSC 5326
Summary
MWSC 5326 is a poorly populated, very loose object of 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) | 248.197 | -17.143 | – | -7.74 | -8.91 | – |
| Bica et al. (2019) | 248.188 | -17.143 | – | – | – | – |
| UCC | 248.191 | -17.162 | 0.276 | -1.69 | -4.168 | -7.529 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.25, distance=1637, log_age=9.485 |
Search coordinates in Bayestar19