CWWDL 13499

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C3
N_50
r_50
CC 11 6.4
Summary

CWWDL 13499 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It was recently reported in the literature.

This is very likely 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=0.92) 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) 318.492 46.149 0.467 -2.87 -3.72
           
UCC 318.425 46.182 0.448 -2.919 -3.73
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWWDL 13499 UCC

Explore data in Colab

Fundamental parameters

Reference Values
Chi et al. (2023) logAge=6.48, Z=0.35

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HXWHB 16 8.0 318.45 46.29 0.57 -2.58 -3.79 -61.77 0.09