CWNU 4850

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.01 0.25 0.0 1.0
C3
N_50
r_50
DB 16 5.9
Summary

CWNU 4850 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, well below 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) 206.395 -66.564 0.115 -5.007 -1.363 –
           
UCC 206.433 -66.568 0.11 -5.025 -1.349 -66.076
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4850 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=0.8, m-M=16.65, logA=9.6

Search coordinates in Bayestar19

Cluster region map