CWNU 1701

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C3
N_50
r_50
DC 21 3.0
Summary

CWNU 1701 is a sparse, 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) 71.812 46.917 0.31 0.657 -1.267 -27.49
           
UCC 71.849 46.931 0.274 0.651 -1.289 -58.654
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1701 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=2.7, m-M=12.0, logAge=8.8

Search coordinates in Bayestar19

Cluster region map