CWNU 4047

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.02 0.25 0.0 0.96
C3
N_50
r_50
DB 16 5.8
Summary

CWNU 4047 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, well above the mid-plane. It was recently reported in the literature.This is a unique object, which shares a very 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=0.96) 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) 320.103 55.469 0.119 -2.53 -2.616 –
           
UCC 320.094 55.457 0.119 -2.511 -2.615 -85.428
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4047 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=4.4, m-M=16.15, logA=6.0

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
BDSB 23 4.0 320.09 55.48 0.15 -2.78 -2.61 -134.33 0.08