MWSC 4218
Summary
MWSC 4218 is a poorly populated, very loose object of very low C3 quality. It is located at a large 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) | 235.11 | -33.475 | – | -5.99 | -7.06 | – |
| Bica et al. (2019) | 235.104 | -33.476 | – | – | – | – |
| UCC | 235.136 | -33.41 | 0.174 | -6.036 | -5.266 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.729, distance=993, log_age=9.1 |
Search coordinates in Bayestar19