CWNU 3433

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C3
N_50
r_50
AC 20 2.7
Summary

CWNU 3433 is a sparse, very loose object of intermediate 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) 108.762 -24.528 0.083 -0.548 1.544 88.17
           
UCC 108.76 -24.528 0.088 -0.506 1.506 84.264
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3433 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=0.85, m-M=14.55, logA=8.8

Search coordinates in Bayestar19

Cluster region map