CWNU 1196

(OCSN 123)

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C3
N_50
r_50
CB 25 38.2
Summary

CWNU 1196 is a poorly populated, loose object of low C3 quality. It is located at a very close distance from the Sun, near the mid-plane. It was recently reported in the literature.

This object shares a large percentage of members with a later reported entry.

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. (2022) 168.537 -70.659 3.449 -21.725 -0.648
Qin et al. (2023) 169.02 -70.85 3.52 -21.99 -1.01 3.7
           
UCC 168.386 -70.638 3.45 -21.725 -0.648 4.719
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1196 UCC

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Fundamental parameters

Reference Values
He et al. (2022) A0=0.6, logAge=7.6
Qin et al. (2023) E(B-V)=0.28, m-M=7.98, logt=7.75

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 2442 100.0 170.96 -71.15 3.49 -21.89 -1.34 4.72 0.19