CWNU 2650

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.34 0.25 0.5 0.0 1.0
C3
N_50
r_50
BB 34 5.3
Summary

CWNU 2650 is a poorly populated, loose object of intermediate C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It was recently reported in the literature.

This object shares a large 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. (2023) 234.812 -58.529 0.299 -3.506 -4.623 -25.44
           
UCC 234.79 -58.542 0.293 -3.502 -4.633 -23.023
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 2650 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=4.0, m-M=12.75, logAge=8.05

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 4482 91.2 234.78 -58.54 0.29 -3.5 -4.64 -23.82 0.07