CWNU 279

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C3
N_50
r_50
CB 22 5.2
Summary

CWNU 279 is a sparse, moderately dense object of low C3 quality. It is located at a relatively close distance from the Sun, near 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) 103.839 -2.151 0.53 -1.42 1.09
Hunt & Reffert (2023) 103.827 -2.132 0.55 -1.401 1.123 29.007
Cavallo et al. (2024) 103.83 -2.151 0.554
Hunt & Reffert (2024) 103.827 -2.132 0.55 -1.401 1.123 29.007
           
UCC 103.831 -2.134 0.537 -1.416 1.093 80.19
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=0.4, m-M=10.85, logAge=7.8, Z=0.008
Hunt & Reffert (2023) AV50=0.293, diffAV50=0.781, MOD50=11.208, logAge50=8.047
Cavallo et al. (2024) AV50=0.04, dMod50=11.16, logAge50=8.34, [Fe/H]50=0.74
Hunt & Reffert (2024) MassJ=91.1505, MassTot=149.393

Search coordinates in Bayestar19

Cluster region map