CWNU 4886

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.0 0.38 0.0 1.0
C3
N_50
r_50
BC 12 4.2
Summary

CWNU 4886 is a sparse, very loose object of low C3 quality. It is located at a very large distance from the Sun, well 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) 292.405 30.163 0.048 -2.082 -3.899 -43.14
           
UCC 292.431 30.168 0.048 -2.105 -3.906 -73.721
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4886 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=0.55, m-M=15.0, logA=10.1

Search coordinates in Bayestar19

Cluster region map