CWNU 4338

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.21 0.38 0.0 1.0
C3
N_50
r_50
BC 23 13.0
Summary

CWNU 4338 is a sparse, very loose object of low C3 quality. It is located at a relatively close distance from the Sun, 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) 103.318 4.728 0.787 -1.724 -2.606 28.4
           
UCC 103.236 4.718 0.805 -1.688 -2.6 40.959
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4338 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.75, m-M=10.55, logA=8.9

Search coordinates in Bayestar19

Cluster region map