FoF 1490
(LP 1490)
Summary
FoF 1490 is a moderately populated, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is rarely studied in the literature.
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) | 157.71 | -58.263 | 0.319 | -6.807 | 3.401 | 0.334 |
| Almeida et al. (2025) | 157.71 | -58.263 | – | – | – | – |
| UCC | 157.755 | -58.238 | 0.334 | -6.817 | 3.4 | 4.109 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2021) | Av=1.05, Dist=2449, logage=7.241, [Fe/H]=0.061 |
| Almeida et al. (2025) | AV=1.05, Dist=2449, logAge=7.241, MassRk=268.6 |
Search coordinates in Bayestar19