CWNU 3273

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C3
N_50
r_50
DB 31 6.4
Summary

CWNU 3273 is a poorly populated, 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 very small percentage of members with at least one previously reported entry.

Warning: the low UTI value and no obvious signs of duplication (C_dup=0.9) 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. (2023) 123.687 -35.69 0.246 -2.952 3.201
           
UCC 123.7 -35.677 0.255 -2.956 3.192
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3273 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=2.35, m-M=12.75, logA=7.1

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
ASCC 45 9.7 124.09 -35.66 0.25 -2.86 3.23 0.62