CWNU 1955

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.17 0.38 0.0 1.0
C3
N_50
r_50
CB 23 4.9
Summary

CWNU 1955 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, below 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) 132.88 -49.442 0.287 -2.773 3.472 -1.09
           
UCC 132.759 -49.355 0.272 -2.775 3.476 3.353
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

CWNU 1955 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=2.6, m-M=13.1, logAge=9.25

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Cluster region map