CWWDL 3447

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C3
N_50
r_50
CC 8 9.9
Summary

CWWDL 3447 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, below the mid-plane. It was recently reported in the literature.

This object shares a very small percentage of members with at least one entry reported in the same catalogue.

Warning: contains less than 25 stars with P>0.5 estimated.

Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) 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) 136.329 -54.445 0.251 -3.709 4.004 28.062
           
UCC 136.294 -54.503 0.199 -3.729 3.975 41.245
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWWDL 3447 UCC

Explore data in Colab

Fundamental parameters

Reference Values
Chi et al. (2023) logAge=8.45, Z=-0.88

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 3434 4.0 136.71 -54.49 0.22 -3.95 3.93 57.64 0.03