CWNU 2365

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C3
N_50
r_50
CC 16 12.8
Summary

CWNU 2365 is a sparse, very loose 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) 343.739 64.736 0.394 -3.359 -1.991 -61.04
           
UCC 343.814 64.722 0.388 -3.334 -1.983 -61.041
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 2365 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=2.55, m-M=11.75, logAge=8.85

Search coordinates in Bayestar19

Cluster region map