CWNU 4888

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C3
N_50
r_50
BB 29 2.9
Summary

CWNU 4888 is a poorly populated, very loose object of intermediate C3 quality. It is located at a very large distance from the Sun, well below the mid-plane. It was recently reported in the literature.

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) 274.567 -32.345 0.058 -3.272 -6.42 -0.08
           
UCC 274.563 -32.362 0.062 -3.255 -6.386 -0.076
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4888 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=0.4, m-M=15.55, logA=9.9

Search coordinates in Bayestar19

Cluster region map