CWNU 1950

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C3
N_50
r_50
CB 16 6.4
Summary

CWNU 1950 is a sparse, very loose object of low C3 quality. It is located at a moderate 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.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2023) 255.482 -28.004 0.451 -2.658 -2.354 35.68
           
UCC 255.473 -28.019 0.442 -2.67 -2.386 -43.02
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1950 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.05, m-M=12.1, logAge=9.45

Search coordinates in Bayestar19

Cluster region map