CWNU 4790

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.02 0.25 0.0 1.0
C3
N_50
r_50
DB 15 3.7
Summary

CWNU 4790 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) 260.808 -23.128 0.112 -3.281 -4.15 –
           
UCC 260.837 -23.107 0.086 -3.29 -4.153 -129.26
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4790 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.35, m-M=16.8, logA=9.4

Search coordinates in Bayestar19

Cluster region map