FoF 1437

(LP 1437)

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C3
N_50
r_50
DC 32 4.6
Summary

FoF 1437 is a poorly populated, very loose object of very low 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 small percentage of members with a later reported entry.

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) 124.115 -33.669 0.246 -2.591 3.033
Dias et al. (2021) 124.106 -33.662 0.237 -2.601 3.041 64.672
Almeida et al. (2025) 124.106 -33.662
           
UCC 124.12 -33.637 0.212 -2.615 3.043 76.945
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

FoF 1437 UCC

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Fundamental parameters

Reference Values
Liu & Pang (2019) Age=0.525, Z=0.5
Dias et al. (2021) Av=1.13, Dist=3631, logage=8.508, [Fe/H]=-0.136
Almeida et al. (2025) AV=1.13, Dist=3631, logAge=8.508, MassRk=4533.8

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 2102 12.5 124.11 -33.59 0.22 -2.49 2.93 0.05