FoF 1370

(LP 1370)

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C3
N_50
r_50
DC 16 5.6
Summary

FoF 1370 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 large 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) 91.432 25.272 0.264 0.297 -1.62
Dias et al. (2021) 91.401 25.253 0.258 0.233 -1.604 18.355
Almeida et al. (2025) 91.401 25.253
           
UCC 91.44 25.238 0.273 0.232 -1.596 68.709
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

FoF 1370 UCC

Explore data in Colab

Fundamental parameters

Reference Values
Liu & Pang (2019) Age=0.576, Z=0.25
Dias et al. (2021) Av=1.183, Dist=3369, logage=8.774, [Fe/H]=-0.113
Almeida et al. (2025) AV=1.183, Dist=3369, logAge=8.774, MassRk=2091.5

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 10817 80.0 91.49 25.3 0.27 0.25 -1.65 45.25 0.11