CWNU 2465

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C3
N_50
r_50
DC 24 8.3
Summary

CWNU 2465 is a sparse, very loose object of very 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 very small percentage of members with at least one entry reported in the same catalogue.

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) 86.988 33.359 0.351 0.398 -1.226
           
UCC 87.0 33.288 0.307 0.388 -1.244 5.521
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 2465 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=1.55, m-M=11.9, logAge=8.55

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2749 8.0 87.28 33.4 0.26 0.14 -1.11 14.99 0.52