CWNU 2212

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C3
N_50
r_50
CC 13 12.3
Summary

CWNU 2212 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.This is a unique object, which shares a very small percentage of members with at least one previously reported entry.

Warning: contains less than 25 stars with P>0.5 estimated.

Warning: the low UTI value and no obvious signs of duplication (C_dup=0.96) 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) 107.916 -8.26 0.354 -1.172 1.653
           
UCC 107.916 -8.254 0.321 -1.172 1.63 61.088
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 2212 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=0.7, m-M=12.0, logAge=9.05

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Dias 3 4.0 107.61 -8.44 0.24 -1.14 1.5 83.29 0.06