CWNU 1785

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C3
N_50
r_50
AA 32 4.1
Summary

CWNU 1785 is a poorly populated, moderately dense object of very high C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It was recently reported in the literature.

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Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2023) 267.864 -27.758 0.333 -0.098 -2.126 -39.69
Hunt & Reffert (2023) 267.901 -27.742 0.336 -0.128 -2.14 -6.559
Cavallo et al. (2024) 267.87 -27.766 0.335
Hunt & Reffert (2024) 267.901 -27.742 0.336 -0.128 -2.14 -6.559
           
UCC 267.847 -27.752 0.334 -0.125 -2.124 -2.481
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=4.4, m-M=12.15, logAge=6.95
Hunt & Reffert (2023) AV50=3.604, diffAV50=2.606, MOD50=12.144, logAge50=7.235
Cavallo et al. (2024) AV50=3.74, dMod50=12.12, logAge50=7.85, [Fe/H]50=-1.04
Hunt & Reffert (2024) MassJ=1001.45, MassTot=1001.45

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Cluster region map