MCM 64
Summary
MCM 64 is a sparse, moderately dense object of intermediate C3 quality. It is located at a moderate 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 2 later reported entries.
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) | 238.907 | -54.644 | – | – | – | – |
| UCC | 238.751 | -54.46 | 0.406 | -3.274 | -3.534 | -34.708 |
Estimated members
Explore data in Colab
Search coordinates in Bayestar19
Cluster region
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Teutsch 246 | 80.0 | 238.7 | -54.39 | 0.41 | -3.27 | -3.53 | -18.97 | 0.67 |
| UBC 1538 | 80.0 | 238.7 | -54.39 | 0.41 | -3.28 | -3.53 | -18.95 | 0.01 |