CWNU 3285

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C3
N_50
r_50
BB 17 7.7
Summary

CWNU 3285 is a sparse, very loose object of intermediate C3 quality. It is located at a large distance from the Sun, 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) 95.099 10.686 0.163 0.07 -0.135 67.51
           
UCC 95.162 10.693 0.177 0.112 -0.134 47.348
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3285 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.95, m-M=14.55, logA=8.4

Search coordinates in Bayestar19

Cluster region map