CWNU 312

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C3
N_50
r_50
AB 36 8.9
Summary

CWNU 312 is a poorly populated, moderately dense object of high C3 quality. It is located at a relatively close distance from the Sun, near the mid-plane. It was recently reported in the literature.

This object shares a large percentage of members with a later reported entry.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2022) 332.496 56.418 0.77 -4.94 -3.83 -23.8
Hunt & Reffert (2023) 332.558 56.469 0.761 -4.951 -3.795 -28.378
Cavallo et al. (2024) 332.307 56.309 0.767
Hunt & Reffert (2024) 332.558 56.469 0.761 -4.951 -3.795 -28.378
           
UCC 332.467 56.385 0.755 -4.944 -3.802 -24.178
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=1.4, m-M=10.85, logAge=8.3, Z=0.036
Hunt & Reffert (2023) AV50=1.424, diffAV50=0.282, MOD50=10.479, logAge50=8.226
Cavallo et al. (2024) AV50=1.69, dMod50=10.67, logAge50=8.31, [Fe/H]50=0.3
Hunt & Reffert (2024) MassJ=131.311, MassTot=189.504

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14215 77.8 332.46 56.38 0.77 -4.94 -3.83 -24.18 0.01