CWNU 2499

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C3
N_50
r_50
DB 36 3.3
Summary

CWNU 2499 is a poorly populated, loose object of low C3 quality. It is located at a moderate distance from the Sun, above 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) 5.42 63.054 0.229 -1.808 -0.606
           
UCC 5.421 63.055 0.222 -1.813 -0.606
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 2499 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=4.0, m-M=13.45, logAge=6.6

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Teutsch J0021.7+6303 97.2 5.42 63.06 0.22 -1.82 -0.61 -128.6 0.02