CWNU 1672

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.09 0.12 0.0 1.0
C3
N_50
r_50
DC 22 13.1
Summary

CWNU 1672 is a sparse, very loose object of very low C3 quality. It is located at a relatively close distance from the Sun, below the mid-plane. It was recently reported in the literature.

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) 91.469 13.887 0.559 1.223 -2.219 28.0
           
UCC 91.514 13.876 0.545 1.24 -2.225 27.999
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1672 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=2.6, m-M=11.5, logAge=8.35

Search coordinates in Bayestar19

Cluster region map