CWNU 4892

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.26 0.03 0.25 0.0 1.0
C3
N_50
r_50
DB 26 6.3
Summary

CWNU 4892 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) 275.988 -28.261 0.143 -3.355 -5.031 -71.84
           
UCC 275.986 -28.273 0.135 -3.359 -5.045 -97.433
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4892 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.1, m-M=13.9, logA=9.5

Search coordinates in Bayestar19

Cluster region map