CWNU 2670

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C3
N_50
r_50
DC 18 5.2
Summary

CWNU 2670 is a sparse, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, above 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) 124.002 -31.295 0.232 -2.399 2.892 107.32
           
UCC 124.074 -31.322 0.223 -2.377 2.879 90.026
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 2670 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=1.65, m-M=13.25, logAge=8.25

Search coordinates in Bayestar19

Cluster region map