FSR 1289
(MWSC 1123)
Summary
FSR 1289 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 poorly 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 |
|---|---|---|---|---|---|---|
| Froebrich et al. (2007) | 107.154 | -26.158 | – | – | – | – |
| Kharchenko et al. (2012) | 107.138 | -26.158 | – | -3.54 | 6.37 | – |
| Bica et al. (2019) | 107.163 | -26.158 | – | – | – | – |
| UCC | 107.101 | -26.094 | 0.195 | -1.168 | 1.782 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.416, distance=1791, log_age=8.605 |
Search coordinates in Bayestar19