CWNU 2495

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C3
N_50
r_50
DB 25 2.3
Summary

CWNU 2495 is a poorly populated, loose object of low C3 quality. It is located at a large distance from the Sun, near the mid-plane. It was recently reported in the literature.

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) 314.819 44.916 0.215 -3.004 -4.098 -39.38
           
UCC 314.819 44.911 0.196 -3.003 -4.097 -39.377
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 2495 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=3.25, m-M=13.0, logAge=8.25

Search coordinates in Bayestar19

Cluster region map