CWNU 1956

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.11 0.75 0.0 1.0
C3
N_50
r_50
AB 22 8.4
Summary

CWNU 1956 is a sparse, very loose object of high 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.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2023) 96.784 2.929 0.373 -0.189 0.025 30.17
           
UCC 96.728 2.88 0.386 -0.194 0.023 25.374
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

CWNU 1956 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.85, m-M=12.6, logAge=8.9

Search coordinates in Bayestar19

Cluster region map