FoF 1956
(LP 1956)
Summary
FoF 1956 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It is rarely studied in the literature.
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 |
|---|---|---|---|---|---|---|
| Dias et al. (2021) | 58.25 | 57.277 | 0.31 | 0.108 | -0.375 | -76.608 |
| Almeida et al. (2025) | 58.25 | 57.277 | – | – | – | – |
| UCC | 58.326 | 57.326 | 0.302 | 0.075 | -0.368 | -52.591 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2021) | Av=1.973, Dist=2966, logage=8.782, [Fe/H]=-0.072 |
| Almeida et al. (2025) | AV=1.973, Dist=2966, logAge=8.782, MassRk=1029.5 |
Search coordinates in Bayestar19