CWNU 264

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C3
N_50
r_50
AC 24 4.9
Summary

CWNU 264 is a sparse, very dense object of intermediate C3 quality. It is located at a relatively close distance from the Sun, below the mid-plane. It was recently reported in the literature.

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) 149.21 -60.52 0.76 -9.28 3.69
Hunt & Reffert (2023) 149.2 -60.53 0.767 -9.321 3.647 -22.985
Cavallo et al. (2024) 149.216 -60.512 0.765
Hunt & Reffert (2024) 149.2 -60.53 0.767 -9.321 3.647 -22.985
           
UCC 149.183 -60.521 0.765 -9.293 3.649 -13.618
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. (2022) AG=0.3, m-M=10.2, logAge=7.6, Z=0.01
Hunt & Reffert (2023) AV50=0.314, diffAV50=0.395, MOD50=10.504, logAge50=7.681
Cavallo et al. (2024) AV50=0.32, dMod50=10.27, logAge50=8.03, [Fe/H]50=-0.38
Hunt & Reffert (2024) MassJ=42.6544, MassTot=84.1774

Search coordinates in Bayestar19

Cluster region map