CWNU 324

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C3
N_50
r_50
AC 44 4.0
Summary

CWNU 324 is a poorly populated, very 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.

Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2022) 113.007 -16.945 0.52 -2.23 2.56
Hunt & Reffert (2023) 113.012 -16.932 0.511 -2.232 2.558 47.015
Cavallo et al. (2024) 113.016 -16.955 0.516
Hunt & Reffert (2024) 113.012 -16.932 0.511 -2.232 2.558 47.015
           
UCC 113.006 -16.942 0.525 -2.207 2.558
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

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Fundamental parameters

Reference Values
He et al. (2022) AG=1.6, m-M=11.95, logAge=6.8, Z=0.02
Hunt & Reffert (2023) AV50=1.229, diffAV50=2.435, MOD50=11.217, logAge50=7.262
Cavallo et al. (2024) AV50=0.93, dMod50=11.59, logAge50=7.39, [Fe/H]50=0.28
Hunt & Reffert (2024) MassJ=446.276, MassTot=388.380

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0394 90.9 113.02 -16.95 0.52 -2.16 2.54 51.1 0.43