CWNU 1730

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C3
N_50
r_50
BB 32 3.3
Summary

CWNU 1730 is a poorly populated, very dense object of intermediate C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It was recently reported in the literature.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2023) 164.68 -60.127 0.385 -6.143 0.818
Hunt & Reffert (2023) 164.698 -60.119 0.389 -6.132 0.819
Cavallo et al. (2024) 164.678 -60.122 0.385
Hunt & Reffert (2024) 164.698 -60.119 0.389 -6.132 0.819
           
UCC 164.687 -60.125 0.389 -6.142 0.813
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.35, m-M=11.9, logAge=8.0
Hunt & Reffert (2023) AV50=0.896, diffAV50=0.775, MOD50=11.88, logAge50=8.166
Cavallo et al. (2024) AV50=1.45, dMod50=11.74, logAge50=7.93, [Fe/H]50=-0.42
Hunt & Reffert (2024) MassJ=181.888, MassTot=202.399

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Cluster region map