CWNU 1188

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C3
N_50
r_50
CB 27 24.3
Summary

CWNU 1188 is a poorly populated, moderately dense object of low C3 quality. It is located at a very close distance from the Sun, above the mid-plane. It was recently reported in the literature.

This object shares a large percentage of members with 2 later reported entries.

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) 269.772 2.899 2.383 0.058 -8.326
           
UCC 269.906 2.931 2.362 0.138 -8.258 -14.985
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1188 UCC

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Fundamental parameters

Reference Values
He et al. (2022) A0=1.05, logAge=7.6

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 305 77.8 269.76 2.93 2.38 0.05 -8.21 -13.41 0.03
HSC 297 3.7 270.7 2.76 1.94 0.42 -8.66 -4.84 0.12