FoF 1332

(LP 1332)

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C3
N_50
r_50
BC 18 7.3
Summary

FoF 1332 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It is poorly studied in the literature.

This object shares a small 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
Liu & Pang (2019) 26.94 60.422 0.321 -0.979 -0.494
Dias et al. (2021) 26.851 60.513 0.316 -1.015 -0.435 -56.742
Almeida et al. (2025) 26.851 60.513
           
UCC 26.929 60.44 0.34 -1.015 -0.471
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

FoF 1332 UCC

Explore data in Colab

Fundamental parameters

Reference Values
Liu & Pang (2019) Age=0.191, Z=0.5
Dias et al. (2021) Av=1.778, Dist=2697, logage=7.773, [Fe/H]=0.051
Almeida et al. (2025) AV=1.778, Dist=2697, logAge=7.773, MassRk=2631.3

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4108 20.0 26.73 60.44 0.36 -1.04 -0.58 0.13