CWNU 1832

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C3
N_50
r_50
BB 29 5.4
Summary

CWNU 1832 is a poorly populated, dense 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) 257.695 -36.015 0.581 1.366 0.443 -29.44
Hunt & Reffert (2023) 257.692 -36.029 0.561 1.334 0.408 -29.454
Cavallo et al. (2024) 257.683 -36.023 0.569
Hunt & Reffert (2024) 257.692 -36.029 0.561 1.334 0.408 -29.454
           
UCC 257.689 -36.028 0.567 1.348 0.441 -29.438
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=3.65, m-M=11.1, logAge=8.15
Hunt & Reffert (2023) AV50=3.436, diffAV50=2.166, MOD50=11.09, logAge50=7.982
Cavallo et al. (2024) AV50=3.65, dMod50=11.0, logAge50=8.09, [Fe/H]50=-0.33
Hunt & Reffert (2024) MassJ=400.383, MassTot=409.432

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Cluster region map