FoF 1355
(LP 1355)
Summary
FoF 1355 is a sparse, moderately dense object of low C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is poorly studied in the literature.
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 |
|---|---|---|---|---|---|---|
| Dias et al. (2021) | 46.023 | 57.774 | 0.323 | -0.235 | -0.381 | -56.181 |
| He et al. (2023) | 46.026 | 57.758 | 0.278 | -0.317 | -0.46 | – |
| Almeida et al. (2025) | 46.023 | 57.774 | – | – | – | – |
| UCC | 46.004 | 57.761 | 0.293 | -0.3 | -0.433 | 2.948 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2021) | Av=2.74, Dist=2731, logage=6.998, [Fe/H]=-0.108 |
| He et al. (2023) | A0=3.35, m-M=12.35, logA=7.5 |
| Almeida et al. (2025) | AV=2.74, Dist=2731, logAge=6.998, MassRk=711.0 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| HSC 1129 | 56.0 | 46.0 | 57.77 | 0.31 | -0.33 | -0.51 | – | 0.23 |