CWNU 260

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C3
N_50
r_50
BB 32 21.1
Summary

CWNU 260 is a poorly populated, loose object of intermediate C3 quality. It is located at a close distance from the Sun, below the mid-plane. It was recently reported in the literature.

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

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2022) 117.435 -49.658 1.3 -4.68 7.85 15.5
Hunt & Reffert (2023) 117.494 -49.718 1.263 -4.738 7.669 15.844
Cavallo et al. (2024) 117.762 -49.712 1.276
Hunt & Reffert (2024) 117.494 -49.718 1.263 -4.738 7.669 15.844
           
UCC 117.471 -49.692 1.306 -4.712 7.787 16.724
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. (2022) AG=0.4, m-M=9.8, logAge=7.9, Z=0.04
Hunt & Reffert (2023) AV50=0.229, diffAV50=0.951, MOD50=9.315, logAge50=8.059
Cavallo et al. (2024) AV50=0.35, dMod50=9.41, logAge50=8.22, [Fe/H]50=0.32
Hunt & Reffert (2024) MassJ=43.3590, MassTot=132.126

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 258 18.8 115.43 -50.08 1.38 -4.52 7.78 16.87 0.15