FoF 1692

(LP 1692)

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C3
N_50
r_50
BA 35 2.0
Summary

FoF 1692 is a poorly populated, very dense object of high 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 large percentage of members with a later reported entry.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2021) 289.171 14.156 0.244 -2.169 -5.371 31.952
He et al. (2023) 289.182 14.164 0.204 -2.156 -5.51 58.43
Almeida et al. (2025) 289.171 14.156
           
UCC 289.178 14.153 0.218 -2.148 -5.452 58.432
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

FoF 1692 UCC

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Fundamental parameters

Reference Values
Dias et al. (2021) Av=2.911, Dist=3926, logage=6.904, [Fe/H]=0.269
He et al. (2023) A0=3.5, m-M=12.85, logA=7.0
Almeida et al. (2025) AV=2.911, Dist=3926, logAge=6.904, MassRk=1578.9

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 407 100.0 289.19 14.16 0.21 -2.16 -5.5 46.67 0.44