CWNU 2387

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.25 0.1 0.25 0.0 1.0
C3
N_50
r_50
CC 25 14.4
Summary

CWNU 2387 is a poorly populated, very loose object of low C3 quality. It is located at a relatively 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. (2023) 89.3 11.016 0.596 -0.92 -2.881 –
           
UCC 89.317 10.987 0.582 -0.943 -2.881 30.303
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 2387 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=0.75, m-M=11.0, logAge=8.65

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 2999 24.0 89.05 11.6 0.6 -0.91 -2.88 8.94 0.07