SAI 105
Summary
SAI 105 is a sparse, very loose object of high C3 quality. It is located at a very large distance from the Sun, below the mid-plane. It is rarely studied in the literature, with no articles listed in the last 6 years.
This object shares a significant 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 |
|---|---|---|---|---|---|---|
| Glushkova et al. (2010) | 137.602 | -49.913 | – | – | – | – |
| Bica et al. (2019) | 137.601 | -49.92 | – | – | – | – |
| UCC | 137.6 | -49.901 | 0.085 | -3.303 | 3.367 | 46.878 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Glushkova et al. (2010) | E(B-V)=1.91, Dist=2950.0, Age=9.05 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 3931 | 64.0 | 137.6 | -49.91 | 0.04 | -3.12 | 3.36 | 46.88 | 0.17 |