MCM 13
Summary
MCM 13 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.
This object shares a large 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) | 283.474 | 0.628 | – | – | – | – |
| UCC | 283.424 | 0.619 | 0.163 | -2.022 | -4.447 | 56.565 |
Estimated members
Explore data in Colab
Search coordinates in Bayestar19
Cluster region
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| GLIMPSE 13 | 76.0 | 283.42 | 0.61 | 0.17 | -1.98 | -4.49 | 56.56 | 0.02 |