CWNU 1952

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.03 0.12 0.0 1.0
C3
N_50
r_50
DC 16 11.8
Summary

CWNU 1952 is a sparse, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, well 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) 285.194 -29.155 0.377 -0.982 -3.625 -17.57
           
UCC 285.214 -29.148 0.34 -0.997 -3.612 32.684
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

CWNU 1952 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=0.55, m-M=11.85, logAge=9.65

Search coordinates in Bayestar19

Cluster region map