CWNU 4461

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C3
N_50
r_50
CB 21 5.0
Summary

CWNU 4461 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) 273.785 -28.506 0.114 -4.453 -6.434 -49.66
           
UCC 273.768 -28.497 0.111 -4.444 -6.433 44.688
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4461 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=0.8, m-M=14.6, logA=9.8

Search coordinates in Bayestar19

Cluster region map