CWNU 3717

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C3
N_50
r_50
CB 22 2.2
Summary

CWNU 3717 is a sparse, loose object of low C3 quality. It is located at a large 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) 18.287 64.51 0.154 -1.746 -0.065
           
UCC 18.288 64.507 0.157 -1.75 -0.084
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3717 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=3.8, m-M=14.5, logA=6.7

Search coordinates in Bayestar19

Cluster region map