CWNU 1722

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C3
N_50
r_50
CB 37 3.8
Summary

CWNU 1722 is a poorly populated, moderately dense object of low C3 quality. It is located at a moderate distance from the Sun, below 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) 8.73 60.605 0.287 -1.596 -0.906
Hunt & Reffert (2023) 8.753 60.566 0.272 -1.623 -0.887 -44.389
Cavallo et al. (2024) 8.727 60.59 0.275
Hunt & Reffert (2024) 8.753 60.566 0.272 -1.623 -0.887 -44.389
           
UCC 8.743 60.595 0.287 -1.614 -0.903
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=2.4, m-M=12.9, logAge=7.45
Hunt & Reffert (2023) AV50=1.816, diffAV50=2.23, MOD50=12.603, logAge50=8.351
Cavallo et al. (2024) AV50=1.64, dMod50=12.75, logAge50=8.37, [Fe/H]50=0.51
Hunt & Reffert (2024) MassJ=320.276, MassTot=416.758

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Cluster region map