FoF 1399

(LP 1399)

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C3
N_50
r_50
DC 17 11.3
Summary

FoF 1399 is a sparse, 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 moderate 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) 107.38 -5.361 0.272 -0.831 0.828
Dias et al. (2021) 107.377 -5.37 0.266 -0.891 0.857
Almeida et al. (2025) 107.377 -5.37
           
UCC 107.305 -5.354 0.245 -0.857 0.839 65.03
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

FoF 1399 UCC

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Fundamental parameters

Reference Values
Liu & Pang (2019) Age=0.661, Z=0.0
Dias et al. (2021) Av=0.866, Dist=3538, logage=8.771, [Fe/H]=-0.119
Almeida et al. (2025) AV=0.866, Dist=3538, logAge=8.771, MassRk=1217.1

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 1398 32.0 107.2 -5.57 0.23 -0.92 0.71 101.08 0.25