CWNU 3117

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.07 0.38 0.0 0.88
C3
N_50
r_50
BC 19 6.1
Summary

CWNU 3117 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It was recently reported in the literature.

This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry.

Warning: contains less than 25 stars with P>0.5 estimated.

Warning: the low UTI value and no obvious signs of duplication (C_dup=0.88) 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) 20.191 65.291 0.249 -1.95 0.041 -75.59
           
UCC 20.223 65.304 0.243 -1.919 0.032 -49.161
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3117 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=2.6, m-M=12.4, logA=8.7

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 1013 12.0 20.83 65.43 0.28 -1.78 0.1 -46.47 0.27