CWWDL 10495

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C3
N_50
r_50
CC 20 6.8
Summary

CWWDL 10495 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 object shares a 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) 7.281 62.986 0.315 -2.777 -0.753 -30.324
           
UCC 7.336 62.967 0.328 -2.742 -0.774 -93.164
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWWDL 10495 UCC

Explore data in Colab

Fundamental parameters

Reference Values
Chi et al. (2023) logAge=7.52, Z=0.44

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 1988 12.0 6.71 62.94 0.36 -2.96 -0.84 -115.41 0.12