CWNU 4058

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.13 0.62 0.0 1.0
C3
N_50
r_50
AC 22 17.7
Summary

CWNU 4058 is a sparse, very loose object of intermediate C3 quality. It is located at a relatively close distance from the Sun, near the mid-plane. It was recently reported in the literature.

This object shares a significant percentage of members with a later 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=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) 73.493 40.443 0.87 1.668 -5.866 -3.03
           
UCC 73.187 40.65 0.88 1.675 -5.874 -3.032
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4058 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=1.25, m-M=10.4, logA=8.3

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 1284 68.0 72.95 40.8 0.9 1.71 -5.88 -6.54 0.06