CWWDL 10380

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C3
N_50
r_50
DC 17 5.3
Summary

CWWDL 10380 is a sparse, very loose object of very 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=0.88) 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) 334.224 56.753 0.237 -3.388 -2.831 -77.715
           
UCC 334.246 56.753 0.231 -3.329 -2.885
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWWDL 10380 UCC

Explore data in Colab

Fundamental parameters

Reference Values
Chi et al. (2023) logAge=8.3, Z=-0.58

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FSR 0356 12.0 334.68 56.77 0.24 -3.18 -2.76 0.13