CWNU 1967

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.25 0.25 0.0 1.0
C3
N_50
r_50
DB 23 6.4
Summary

CWNU 1967 is a sparse, loose object of low C3 quality. It is located at a moderate distance from the Sun, near 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) 300.907 28.816 0.438 -2.334 -5.359 –
           
UCC 300.899 28.845 0.436 -2.325 -5.341 12.732
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

CWNU 1967 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=3.9, m-M=11.9, logAge=6.45

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Cluster region map