CWNU 4880

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C3
N_50
r_50
AB 29 3.4
Summary

CWNU 4880 is a poorly populated, very loose object of high 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) 267.641 -36.554 0.072 -2.408 -4.678
           
UCC 267.617 -36.558 0.078 -2.419 -4.681 -73.303
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4880 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=2.2, m-M=15.6, logA=9.1

Search coordinates in Bayestar19

Cluster region map