FoF 1595

(LP 1595)

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C3
N_50
r_50
DC 10 9.0
Summary

FoF 1595 is a sparse, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is rarely studied in the literature.

This object shares a small percentage of members with 2 later reported entries.

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
Dias et al. (2021) 185.574 -62.513 0.274 -6.622 0.375
Almeida et al. (2025) 185.574 -62.513
           
UCC 185.662 -62.433 0.253 -6.617 0.379 -25.579
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

FoF 1595 UCC

Explore data in Colab

Fundamental parameters

Reference Values
Dias et al. (2021) Av=2.301, Dist=3413, logage=8.025, [Fe/H]=0.082
Almeida et al. (2025) AV=2.301, Dist=3413, logAge=8.025, MassRk=1700.9

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 2506 16.0 185.53 -62.31 0.24 -6.49 0.42 31.11 0.34
CWNU 3787 8.0 185.53 -62.31 0.24 -6.49 0.41 72.51 0.0