CWWDL 10272

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C3
N_50
r_50
DC 19 6.7
Summary

CWWDL 10272 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 is very likely a unique object, which shares a small percentage of members with at least one previously reported entry, and a small percentage 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=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) 302.911 36.553 0.377 -2.772 -5.698
           
UCC 302.891 36.573 0.415 -2.782 -5.699 -2.17
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWWDL 10272 UCC

Explore data in Colab

Fundamental parameters

Reference Values
Chi et al. (2023) logAge=5.78, Z=0.44

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 10273 12.0 302.87 36.5 0.43 -2.51 -5.61 0.06
CWWDL 13929 12.0 302.83 36.51 0.45 -2.62 -5.79 -28.41 0.09
UBC 368 12.0 302.86 36.51 0.44 -2.57 -5.78 -42.81 0.59