FoF 1831

(LP 1831)

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C3
N_50
r_50
BC 17 7.1
Summary

FoF 1831 is a sparse, very loose object of 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 very 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) 359.239 63.481 0.249 -2.606 -0.893
Dias et al. (2021) 359.192 63.466 0.241 -2.64 -0.906 -72.454
Almeida et al. (2025) 359.192 63.466
           
UCC 359.166 63.499 0.233 -2.641 -0.899
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

FoF 1831 UCC

Explore data in Colab

Fundamental parameters

Reference Values
Liu & Pang (2019) Age=0.468, Z=0.25
Dias et al. (2021) Av=2.031, Dist=3315, logage=7.203, [Fe/H]=0.133
Almeida et al. (2025) AV=2.031, Dist=3315, logAge=7.203, MassRk=796.0

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 10461 4.0 359.47 63.83 0.26 -2.43 -0.95 -89.84 0.03