CWNU 2697

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C3
N_50
r_50
DC 31 14.8
Summary

CWNU 2697 is a poorly populated, 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: 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) 96.873 1.571 0.521 -0.212 -1.498
           
UCC 96.846 1.553 0.507 -0.21 -1.5
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 2697 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=1.85, m-M=11.15, logAge=8.35

Search coordinates in Bayestar19

Cluster region map