SAI 112
Summary
SAI 112 is a sparse, very loose object of very low C3 quality. It is located at a 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.
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) | 155.354 | -59.093 | – | – | – | – |
| Bica et al. (2019) | 155.351 | -59.094 | – | – | – | – |
| UCC | 155.366 | -59.11 | 0.159 | -5.599 | 2.855 | 7.235 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Glushkova et al. (2010) | E(B-V)=1.0, Dist=7240.0, Age=9.1 |
Search coordinates in Bayestar19