FoF 1414

(LP 1414)

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C3
N_50
r_50
BB 20 4.2
Summary

FoF 1414 is a sparse, very loose object of intermediate C3 quality. It is located at a moderate distance from the Sun, above 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) 116.418 -19.138 0.251 -1.841 2.264
He et al. (2023) 116.41 -19.181 0.237 -1.677 2.199
Almeida et al. (2025) 116.418 -19.138
           
UCC 116.441 -19.167 0.243 -1.723 2.244
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

FoF 1414 UCC

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Fundamental parameters

Reference Values
Dias et al. (2021) Av=1.221, Dist=3445, logage=7.938, [Fe/H]=-0.101
He et al. (2023) A0=0.75, m-M=12.7, logA=8.7
Almeida et al. (2025) AV=1.221, Dist=3445, logAge=7.938, MassRk=1244.9

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 1876 56.0 116.44 -19.19 0.26 -1.68 2.21 0.16