CWWDL 4607

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C3
N_50
r_50
AB 23 9.2
Summary

CWWDL 4607 is a sparse, very 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 a unique object, which shares a very small percentage of members with at least one previously reported entry, and a significant percentage 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=0.96) 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) 33.986 57.725 0.41 -0.832 -1.067
           
UCC 33.957 57.708 0.414 -0.822 -1.042 317.007
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWWDL 4607 UCC

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Fundamental parameters

Reference Values
Chi et al. (2023) logAge=6.45, Z=0.2

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 13364 56.0 34.05 57.8 0.43 -0.84 -1.05 317.01 0.14
UBC 46 4.0 33.69 57.31 0.4 -0.83 -1.16 13.37 0.27