CWNU 4270

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.36 0.06 0.25 0.0 1.0
C3
N_50
r_50
CC 36 4.1
Summary

CWNU 4270 is a poorly populated, very loose object of low C3 quality. It is located at a large distance from the Sun, well below the mid-plane. It was recently reported in the literature.

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. (2023) 140.88 -56.073 0.132 -3.371 3.214 –
           
UCC 140.885 -56.077 0.113 -3.374 3.211 55.098
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4270 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.55, m-M=14.9, logA=8.9

Search coordinates in Bayestar19

Cluster region map