CWWDL 10490

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C3
N_50
r_50
DC 17 6.3
Summary

CWWDL 10490 is a sparse, very loose object of very 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 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) 13.336 63.728 0.243 -1.823 -0.384 -54.925
           
UCC 13.319 63.704 0.232 -1.858 -0.335 -87.467
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWWDL 10490 UCC

Explore data in Colab

Fundamental parameters

Reference Values
Chi et al. (2023) logAge=8.06, Z=0.12

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 10477 12.0 12.92 63.82 0.24 -1.76 -0.3 -80.39 0.12