Cmg 903
Summary
Cmg 903 is a sparse, very loose object of very low C3 quality. It is located at a large distance from the Sun, well below the mid-plane. It is rarely studied in the literature, with no articles listed in the last 6 years.
This object shares a moderate percentage of members with at least one entry reported in the same catalogue.
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 |
|---|---|---|---|---|---|---|
| Bica et al. (2019) | 64.001 | 32.312 | – | – | – | – |
| UCC | 63.981 | 32.292 | 0.158 | -0.102 | -0.958 | -19.146 |
Estimated members
Explore data in Colab
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Cmg 902 | 40.0 | 63.78 | 32.25 | 0.21 | -0.05 | -0.46 | -17.91 | 0.29 |
| HSC 1293 | 4.0 | 63.79 | 32.27 | 0.19 | 0.26 | -0.66 | -12.1 | 0.04 |