MWSC 4622
Summary
MWSC 4622 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) | 321.51 | -17.75 | – | 2.27 | -8.49 | – |
| Bica et al. (2019) | 321.517 | -17.748 | – | – | – | – |
| UCC | 321.524 | -17.766 | 0.329 | -2.44 | -4.933 | -31.553 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.208, distance=1075, log_age=9.3 |
Search coordinates in Bayestar19