CWWDL 10399

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C3
N_50
r_50
CC 14 9.4
Summary

CWWDL 10399 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 is very likely a unique object, which shares a small percentage of members with at least one previously reported entry.

Warning: contains less than 25 stars with P>0.5 estimated.

Warning: the low UTI value and no obvious signs of duplication (C_dup=0.84) 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) 351.055 61.275 0.285 -3.815 -1.785 -54.102
           
UCC 351.286 61.32 0.293 -3.852 -1.839 -58.12
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWWDL 10399 UCC

Explore data in Colab

Fundamental parameters

Reference Values
Chi et al. (2023) logAge=7.82, Z=0.44

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 399 16.0 351.34 61.33 0.37 -4.01 -2.15 -57.18 0.2