CWNU 3747

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C3
N_50
r_50
CC 19 4.7
Summary

CWNU 3747 is a sparse, very loose object of low C3 quality. It is located at a large 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) 191.654 -67.965 0.162 -7.253 -0.429
           
UCC 191.682 -67.956 0.152 -7.239 -0.43 -27.546
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3747 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=1.75, m-M=13.95, logA=9.1

Search coordinates in Bayestar19

Cluster region map