CWWDL 2102

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C3
N_50
r_50
CC 10 8.1
Summary

CWWDL 2102 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 was recently reported in the literature.

This is very likely a unique object, which shares a 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=0.84) 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) 124.077 -33.578 0.263 -2.48 2.955 57.644
           
UCC 124.115 -33.589 0.223 -2.489 2.928
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWWDL 2102 UCC

Explore data in Colab

Fundamental parameters

Reference Values
Chi et al. (2023) logAge=7.79, Z=0.4

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 1437 16.0 124.12 -33.64 0.21 -2.62 3.04 76.94 0.22