CWWDL 2690

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C3
N_50
r_50
BC 18 8.3
Summary

CWWDL 2690 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, above 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) 118.887 -24.008 0.271 -2.264 2.911 63.118
           
UCC 118.865 -24.014 0.247 -2.246 2.893 105.923
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWWDL 2690 UCC

Explore data in Colab

Fundamental parameters

Reference Values
Chi et al. (2023) logAge=8.06, Z=-0.58

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 2693 8.0 118.67 -24.07 0.23 -2.54 3.04 113.91 0.06