CWNU 1947

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C3
N_50
r_50
CC 17 9.1
Summary

CWNU 1947 is a sparse, very loose object of low C3 quality. It is located at a relatively close 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) 285.348 -29.394 0.53 -1.207 -2.867 -24.65
           
UCC 285.37 -29.356 0.519 -1.229 -2.87 -23.265
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1947 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=0.5, m-M=11.85, logAge=9.5

Search coordinates in Bayestar19

Cluster region map