CWNU 3917

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.38 0.18 0.38 0.0 1.0
C3
N_50
r_50
BC 38 4.2
Summary

CWNU 3917 is a poorly populated, very 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: 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) 17.87 68.257 0.175 -2.221 0.482 -73.86
           
UCC 17.893 68.266 0.188 -2.211 0.41 -73.863
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3917 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=2.55, m-M=13.2, logA=9.1

Search coordinates in Bayestar19

Cluster region map