CWNU 3443

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.27 0.84 0.38 0.0 0.82
C3
N_50
r_50
BC 27 1.9
Summary

CWNU 3443 is a poorly populated, dense 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 small percentage of members with at least one previously reported entry.

Warning: the low UTI value and no obvious signs of duplication (C_dup=0.82) 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) 112.871 -20.418 0.245 -1.151 2.181 –
           
UCC 112.872 -20.414 0.218 -1.122 2.175 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3443 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.4, m-M=13.35, logA=8.9

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Alessi 192 18.5 112.98 -20.34 0.22 -1.08 2.45 – 0.03