MCM 58
Summary
MCM 58 is a sparse, very loose object of low 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 significant 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) | 225.83 | -58.602 | – | – | – | – |
| UCC | 226.096 | -58.535 | 0.346 | -5.059 | -3.398 | -2.928 |
Estimated members
Explore data in Colab
Search coordinates in Bayestar19
Cluster region
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| FoF 265 | 56.0 | 226.18 | -58.49 | 0.3 | -4.94 | -3.48 | -62.07 | 0.59 |
| HSC 2679 | 24.0 | 226.18 | -58.49 | 0.29 | -5.0 | -3.47 | -62.78 | 0.0 |