CWNU 4856

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.08 0.12 0.0 1.0
C3
N_50
r_50
DC 22 5.8
Summary

CWNU 4856 is a sparse, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It was recently reported in the literature.

This object shares a very small percentage of members with at least one entry reported in the same catalogue.

Warning: contains less than 25 stars with P>0.5 estimated.

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) 168.232 -67.769 0.23 -5.493 1.808 -21.62
           
UCC 168.232 -67.751 0.233 -5.519 1.775 -21.621
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4856 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=0.2, m-M=13.55, logA=10.1

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3593 4.0 167.91 -67.89 0.08 -5.17 1.97 6.51 0.24