CWNU 4637

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C3
N_50
r_50
BB 24 6.6
Summary

CWNU 4637 is a sparse, very loose object of intermediate C3 quality. It is located at a large 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) 278.806 -13.544 0.159 -2.769 -5.252 1.82
           
UCC 278.832 -13.518 0.117 -2.791 -5.261 112.827
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4637 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=3.4, m-M=14.55, logA=9.1

Search coordinates in Bayestar19

Cluster region map