CWNU 1759

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C3
N_50
r_50
BB 26 8.6
Summary

CWNU 1759 is a poorly populated, very loose object of intermediate C3 quality. It is located at a relatively close distance from the Sun, above 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) 169.176 -59.62 0.525 -6.524 1.413
Hunt & Reffert (2023) 169.301 -59.639 0.518 -6.502 1.433 -20.224
Cavallo et al. (2024) 169.075 -59.606 0.519
Hunt & Reffert (2024) 169.301 -59.639 0.518 -6.502 1.433 -20.224
           
UCC 169.038 -59.604 0.518 -6.524 1.425 -20.16
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=1.3, m-M=11.3, logAge=8.6
Hunt & Reffert (2023) AV50=1.036, diffAV50=0.99, MOD50=11.293, logAge50=8.238
Cavallo et al. (2024) AV50=1.43, dMod50=11.41, logAge50=8.23, [Fe/H]50=-0.08
Hunt & Reffert (2024) MassJ=173.013, MassTot=215.571

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Cluster region map