CWNU 4028

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.02 0.38 0.0 0.92
C3
N_50
r_50
BC 16 4.7
Summary

CWNU 4028 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, below the mid-plane. It was recently reported in the literature.

This is very likely a unique object, which shares a very small percentage of members with at least one previously reported entry.

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

Warning: the low UTI value and no obvious signs of duplication (C_dup=0.92) 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) 101.983 -6.285 0.114 -0.173 0.604 74.82
           
UCC 102.001 -6.296 0.106 -0.186 0.56 61.529
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4028 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.55, m-M=14.15, logA=8.4

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 1726 8.0 101.88 -6.38 0.13 -0.37 0.53 – 0.56