CWNU 1948

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C3
N_50
r_50
DB 17 8.0
Summary

CWNU 1948 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) 256.362 -27.929 0.404 -0.755 -3.018
           
UCC 256.31 -27.885 0.386 -0.749 -3.032 -51.014
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1948 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=2.0, m-M=12.5, logAge=9.25

Search coordinates in Bayestar19

Cluster region map