CWNU 270

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C3
N_50
r_50
DB 23 41.4
Summary

CWNU 270 is a sparse, very loose object of low C3 quality. It is located at a close distance from the Sun, below the mid-plane. It was recently reported in the literature.

This object shares a very small percentage of members with a later 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=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. (2022) 108.882 -52.303 1.7 -4.23 8.71 4.6
           
UCC 109.016 -52.222 1.679 -4.243 8.601 15.019
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 270 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2022) AG=0.25, m-M=8.8, logAge=8.0, Z=0.02

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 649 4.0 112.56 -51.37 1.53 -4.39 8.45 12.83 0.07