CWNU 294

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C3
N_50
r_50
AB 36 42.6
Summary

CWNU 294 is a poorly populated, very loose object of high 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 moderate percentage of members with at least one entry reported in the same catalogue.

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) 334.857 43.136 1.59 -0.98 -4.4 -8.0
           
UCC 334.609 42.995 1.591 -0.976 -4.382 -8.62
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 294 UCC

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Fundamental parameters

Reference Values
He et al. (2022) AG=0.45, m-M=8.5, logAge=7.6, Z=0.012

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 237 30.6 335.89 43.28 1.64 -0.83 -4.53 -8.8 0.12
CWNU 311 22.2 332.91 42.37 1.56 -1.14 -4.52 -10.47 0.25