CWNU 4891

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C3
N_50
r_50
DC 15 6.4
Summary

CWNU 4891 is a sparse, very loose object of very low C3 quality. It is located at a large distance from the Sun, 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) 273.307 -5.933 0.2 -2.151 -4.462
           
UCC 273.283 -5.961 0.191 -2.129 -4.395 -12.079
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4891 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=3.05, m-M=14.65, logA=9.6

Search coordinates in Bayestar19

Cluster region map