CWNU 1077

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C3
N_50
r_50
DB 51 269.5
Summary

CWNU 1077 is a moderately 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 small 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) 11.266 2.144 8.376 17.273 -13.475
           
UCC 9.495 1.899 8.434 17.548 -14.392 15.682
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1077 UCC

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Fundamental parameters

Reference Values
He et al. (2022) A0=0.35, logAge=8.0

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 749 23.5 6.06 2.71 8.23 18.26 -14.78 12.49 0.06