CWWDL 13327

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.07 0.25 0.0 0.96
C3
N_50
r_50
CC 18 9.9
Summary

CWWDL 13327 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It was recently reported in the literature.This is a unique object, which shares a very small percentage of members with at least one previously 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=0.96) 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
Chi et al. (2023) 115.629 -27.936 0.451 -2.243 2.264 –
           
UCC 115.701 -27.878 0.41 -2.266 2.265 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWWDL 13327 UCC

Explore data in Colab

Fundamental parameters

Reference Values
Chi et al. (2023) logAge=8.09, Z=-0.88

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 1957 8.0 115.78 -28.16 0.34 -2.36 2.41 102.04 0.24
Teutsch 212 4.0 115.71 -27.41 0.35 -2.27 2.3 – 0.07