CWNU 2492

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.28 0.12 0.0 1.0
C3
N_50
r_50
DC 18 8.1
Summary

CWNU 2492 is a sparse, loose object of very 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.

Warning: contains less than 25 stars with P>0.5 estimated.

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) 309.575 35.101 0.684 -2.937 -5.32 –
           
UCC 309.646 35.077 0.657 -2.957 -5.319 -39.372
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 2492 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=2.05, m-M=10.8, logAge=7.5

Search coordinates in Bayestar19

Cluster region map