MCM 91
Summary
MCM 91 is a sparse, very dense object of low C3 quality. It is located at a relatively close 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 very small percentage of members with a later reported entry.
Warning: contains less than 25 stars with P>0.5 estimated.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Mercer et al. (2005) | 258.11 | -38.524 | – | – | – | – |
| UCC | 258.094 | -38.515 | 0.513 | -1.024 | -2.385 | 11.102 |
Estimated members
Explore data in Colab
Search coordinates in Bayestar19
Cluster region
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Ryu 401 | 8.0 | 257.95 | -38.61 | 0.66 | -1.41 | -3.07 | -39.66 | 0.23 |