CWWDL 12507

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C3
N_50
r_50
BC 17 7.4
Summary

CWWDL 12507 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) 78.115 45.395 0.286 0.76 -1.523 -41.04
           
UCC 78.105 45.33 0.286 0.667 -1.482 -7.563
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWWDL 12507 UCC

Explore data in Colab

Fundamental parameters

Reference Values
Chi et al. (2023) logAge=7.85, Z=-0.28

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2505 16.0 78.06 45.31 0.29 0.49 -1.33 -40.34 0.13