CWNU 1124

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.06 0.12 0.0 0.8
C3
N_50
r_50
DC 21 78.6
Summary

CWNU 1124 is a sparse, very loose object of very low C3 quality. It is located at a very close distance from the Sun, near the mid-plane. It was recently reported in the literature.

This is very likely a unique object, which shares a small percentage of members with at least one previously 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=0.8) 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) 324.639 50.397 2.855 7.069 1.839 –
           
UCC 324.767 50.258 2.83 7.142 1.765 -16.919
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1124 UCC

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Fundamental parameters

Reference Values
He et al. (2022) A0=0.35, logAge=7.75

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
NGC 7058 20.0 320.47 50.82 2.73 7.45 2.75 -19.44 1.0