FoF 1355

(LP 1355)

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C3
N_50
r_50
CC 22 2.8
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.

Search object in SciX | Simbad

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
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

FoF 1355 UCC

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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