CWWDL 232

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C3
N_50
r_50
AB 21 4.5
Summary

CWWDL 232 is a sparse, loose object of high 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 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) 34.359 56.636 0.374 -0.678 -1.153 -33.592
           
UCC 34.399 56.661 0.386 -0.681 -1.203
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWWDL 232 UCC

Explore data in Colab

Fundamental parameters

Reference Values
Chi et al. (2023) logAge=6.28, Z=0.4

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0247 16.0 34.61 56.85 0.38 -0.62 -1.18 0.16