CWNU 3090

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C3
N_50
r_50
CC 22 3.3
Summary

CWNU 3090 is a sparse, moderately dense object of low C3 quality. It is located at a moderate 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) 103.748 16.041 0.353 1.122 -1.844 43.12
           
UCC 103.74 16.052 0.342 1.114 -1.841 43.116
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3090 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=0.95, m-M=12.55, logA=8.7

Search coordinates in Bayestar19

Cluster region map