CWNU 539

(OCSN 161)

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C3
N_50
r_50
CB 30 31.5
Summary

CWNU 539 is a poorly populated, loose object of low C3 quality. It is located at a very close distance from the Sun, below the mid-plane. It was recently reported in the literature.

This object shares a large percentage of members with a later reported entry.

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) 103.814 -37.54 2.22 -8.94 10.48 27.1
Qin et al. (2023) 103.83 -37.6 2.18 -8.61 10.32 28.63
           
UCC 103.785 -37.565 2.227 -8.944 10.485 29.394
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 539 UCC

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Fundamental parameters

Reference Values
He et al. (2022) AG=0.2, m-M=7.8, logAge=7.7, Z=0.006
Qin et al. (2023) E(B-V)=0.17, m-M=8.74, logt=8.4

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 249 80.0 103.76 -37.56 2.23 -8.87 10.52 28.76 0.02