CWNU 1091

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C3
N_50
r_50
DB 27 127.8
Summary

CWNU 1091 is a poorly populated, very loose object of low C3 quality. It is located at a very close distance from the Sun, below the mid-plane. It was recently reported in the literature.

This object shares a significant percentage of members with a later reported entry.

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) 332.61 12.116 5.238 14.904 -10.696
           
UCC 333.23 12.605 5.255 15.085 -10.85 -2.469
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1091 UCC

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Fundamental parameters

Reference Values
He et al. (2022) A0=0.25, logAge=8.1

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 598 59.3 335.01 13.29 5.31 15.51 -11.2 5.54 0.06