MCM 18
Summary
MCM 18 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, near the mid-plane. It is rarely studied in the literature, with no articles listed in the last 20 years.
Warning: contains less than 25 stars with P>0.5 estimated.
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 |
|---|---|---|---|---|---|---|
| Mercer et al. (2005) | 287.46 | 8.325 | – | – | – | – |
| UCC | 287.44 | 8.252 | 0.106 | -2.171 | -5.353 | 55.872 |
Estimated members
Explore data in Colab
Search coordinates in Bayestar19