CWNU 3392

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.08 0.12 0.0 1.0
C3
N_50
r_50
DC 21 1.9
Summary

CWNU 3392 is a sparse, very loose object of very low 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: 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) 133.662 -58.262 0.075 -2.549 3.323 19.12
           
UCC 133.658 -58.252 0.075 -2.618 3.272 19.117
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3392 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=0.35, m-M=15.0, logA=9.6

Search coordinates in Bayestar19

Cluster region map