CWNU 1732

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.25 0.62 0.0 1.0
C3
N_50
r_50
AC 23 10.4
Summary

CWNU 1732 is a sparse, loose object of intermediate C3 quality. It is located at a relatively close distance from the Sun, above the mid-plane. It was recently reported in the literature.

This object shares a large 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) 81.155 38.234 0.708 2.316 -5.83 -9.02
           
UCC 81.174 38.242 0.706 2.317 -5.825 -9.953
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1732 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=0.95, m-M=10.65, logAge=8.75

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 1424 92.0 81.2 38.24 0.7 2.33 -5.82 -9.95 0.03