CWNU 4457

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.25 0.27 0.25 0.0 1.0
C3
N_50
r_50
DB 25 4.5
Summary

CWNU 4457 is a poorly populated, loose object of low C3 quality. It is located at a moderate distance from the Sun, 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) 38.968 58.563 0.296 -0.314 -0.808 -73.9
           
UCC 38.979 58.539 0.303 -0.297 -0.799 -73.905
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4457 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=3.05, m-M=12.35, logA=8.6

Search coordinates in Bayestar19

Cluster region map