CWNU 1993

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.41 0.12 0.0 1.0
C3
N_50
r_50
DC 20 8.1
Summary

CWNU 1993 is a sparse, loose object of very low C3 quality. It is located at a relatively close 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.

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Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2023) 312.251 55.473 0.755 -1.417 -3.976 -8.73
           
UCC 312.151 55.51 0.75 -1.417 -3.971 -8.731
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

CWNU 1993 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.9, m-M=10.5, logAge=8.35

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Cluster region map