MCM 11
Summary
MCM 11 is a sparse, very loose object of very 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.
This object shares a small percentage of members with a later reported entry.
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) | 281.674 | -2.736 | – | – | – | – |
| UCC | 281.659 | -2.771 | 0.184 | -1.144 | -3.823 | – |
Estimated members
Explore data in Colab
Search coordinates in Bayestar19
Cluster region
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| BDSB 125 | 24.0 | 281.46 | -2.73 | 0.24 | -1.17 | -3.72 | 28.11 | 0.19 |