CWNU 2396

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C3
N_50
r_50
BC 14 6.5
Summary

CWNU 2396 is a sparse, very 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 small percentage of members with a later reported entry.

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) 326.469 55.443 0.372 -2.714 -2.681 -38.92
           
UCC 326.482 55.49 0.371 -2.699 -2.685
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 2396 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=1.9, m-M=12.4, logAge=6.45

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 772 16.0 326.5 55.58 0.18 -2.8 -2.7 0.16