CWNU 4887

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.32 0.08 0.5 0.0 1.0
C3
N_50
r_50
BB 32 2.5
Summary

CWNU 4887 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) 270.657 -29.77 0.081 -3.626 -6.476 –
           
UCC 270.664 -29.77 0.083 -3.664 -6.451 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4887 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=1.15, m-M=17.2, logA=8.9

Search coordinates in Bayestar19

Cluster region map