CWNU 512

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C3
N_50
r_50
CB 22 24.0
Summary

CWNU 512 is a sparse, very loose object of low C3 quality. It is located at a close distance from the Sun, above the mid-plane. It was recently reported in the literature.

This object shares a large percentage of members with at least one entry reported in the same catalogue.

Warning: contains less than 25 stars with P>0.5 estimated.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2022) 6.213 68.937 1.05 -2.8 -0.01
Hunt & Reffert (2023) 5.095 68.734 1.046 -2.845 -0.155 -23.788
Cavallo et al. (2024) 4.603 68.921 1.044
Hunt & Reffert (2024) 5.095 68.734 1.046 -2.845 -0.155 -23.788
           
UCC 5.086 68.902 1.05 -2.847 -0.142 -21.482
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2022) AG=2.2, m-M=10.9, logAge=6.5, Z=0.002
Hunt & Reffert (2023) AV50=2.929, diffAV50=1.845, MOD50=9.779, logAge50=7.97
Cavallo et al. (2024) AV50=3.03, dMod50=10.22, logAge50=7.55, [Fe/H]50=0.21
Hunt & Reffert (2024) MassJ=70.4268, MassTot=147.849

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 343 84.0 4.53 68.9 1.05 -2.85 -0.19 -23.56 0.14