CWNU 3440

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C3
N_50
r_50
BC 24 2.4
Summary

CWNU 3440 is a sparse, loose object of low C3 quality. It is located at a moderate distance from the Sun, well 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) 31.634 67.983 0.23 -0.86 0.419
           
UCC 31.63 67.983 0.206 -0.893 0.377
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3440 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=2.45, m-M=13.75, logA=9.3

Search coordinates in Bayestar19

Cluster region map