CWNU 1239

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C3
N_50
r_50
AC 18 18.6
Summary

CWNU 1239 is a sparse, very loose object of intermediate C3 quality. It is located at a close distance from the Sun, near the mid-plane. It was recently reported in the literature.

This is very likely a unique object, which shares a small percentage of members with at least one previously 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=0.84) 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. (2022) 130.232 -40.792 1.079 -5.404 3.465
           
UCC 129.848 -40.539 1.059 -5.385 3.468 -15.306
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1239 UCC

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Fundamental parameters

Reference Values
He et al. (2022) A0=0.3, logAge=6.5

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 2221 16.0 129.43 -40.23 1.06 -5.62 3.77 21.57 0.41
OC 0467 16.0 129.4 -40.29 1.06 -5.67 3.69 19.99 0.09
OC 0472 16.0 130.27 -40.83 1.07 -4.96 3.2 12.76 0.42