CWWDL 4776

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C3
N_50
r_50
CC 27 8.7
Summary

CWWDL 4776 is a poorly populated, 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 a unique object, which shares a very small percentage of members with at least one previously reported entry.

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) 116.502 -26.629 0.324 -2.177 2.536
           
UCC 116.509 -26.629 0.31 -2.198 2.557
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWWDL 4776 UCC

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Fundamental parameters

Reference Values
Chi et al. (2023) logAge=7.7, Z=0.4

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3133 3.7 116.49 -26.7 0.33 -2.08 2.28 53.55 0.04
HSC 1946 3.7 116.48 -26.7 0.33 -2.08 2.27 53.55 0.25
UBC 1394 3.7 116.46 -26.6 0.29 -2.24 2.81 0.39