CWNU 1928

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.17 0.25 0.0 1.0
C3
N_50
r_50
DB 19 6.2
Summary

CWNU 1928 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, near 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) 148.154 -54.493 0.383 -5.876 3.462 –
           
UCC 148.189 -54.514 0.379 -5.876 3.465 43.403
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1928 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.25, m-M=12.0, logAge=6.95

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1629 8.0 148.29 -54.2 0.4 -6.0 3.44 43.4 0.11