CWNU 1962

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C3
N_50
r_50
CC 23 5.2
Summary

CWNU 1962 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, near 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) 108.47 -10.52 0.332 -0.563 0.213 58.64
Hunt & Reffert (2023) 108.477 -10.52 0.336 -0.587 0.215
Hunt & Reffert (2024) 108.477 -10.52 0.336 -0.587 0.215
           
UCC 108.459 -10.524 0.33 -0.575 0.213 58.642
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.5, m-M=12.5, logAge=8.8
Hunt & Reffert (2023) AV50=1.184, diffAV50=0.512, MOD50=12.265, logAge50=8.657
Hunt & Reffert (2024) MassJ=204.019, MassTot=204.019

Search coordinates in Bayestar19

Cluster region map