CWNU 4571

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.04 0.12 0.0 1.0
C3
N_50
r_50
DC 19 6.5
Summary

CWNU 4571 is a sparse, very loose object of very 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.

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) 104.359 14.816 0.179 -0.132 -0.616 -0.76
           
UCC 104.335 14.799 0.187 -0.153 -0.586 -0.763
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4571 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=0.45, m-M=14.25, logA=9.1

Search coordinates in Bayestar19

Cluster region map