CWNU 533

(OCSN 110)

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C3
N_50
r_50
CB 22 49.2
Summary

CWNU 533 is a sparse, very loose object of low C3 quality. It is located at a very close distance from the Sun, near the mid-plane. It was recently reported in the literature.

This object shares a large percentage of members with a later 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=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
He et al. (2022) 358.114 55.399 2.24 5.29 -4.55 -12.5
He et al. (2022) 356.947 54.996 2.362 5.246 -4.441
Qin et al. (2023) 356.19 54.99 2.28 5.28 -4.47 -13.41
           
UCC 357.124 55.144 2.271 5.253 -4.463 -13.415
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 533 UCC

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Fundamental parameters

Reference Values
He et al. (2022) AG=0.95, m-M=8.85, logAge=7.7, Z=0.028
He et al. (2022) A0=0.8, logAge=7.9
Qin et al. (2023) E(B-V)=0.28, m-M=8.98, logt=7.9

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 391 100.0 356.34 55.15 2.25 5.13 -4.41 -13.09 0.25