CWNU 1712

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.63 0.12 0.42 1.0
C3
N_50
r_50
DC 23 6.8
Summary

CWNU 1712 is a sparse, moderately dense object of very 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.

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Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2023) 106.53 -6.367 0.726 -1.385 0.632 –
Hunt & Reffert (2023) 106.551 -6.36 0.739 -1.395 0.65 5.767
Cavallo et al. (2024) 106.548 -6.363 0.735 – – –
Hunt & Reffert (2024) 106.551 -6.36 0.739 -1.395 0.65 5.767
Hu & Soubiran (2025) 106.548 -6.363 – – – –
           
UCC 106.535 -6.363 0.729 -1.397 0.638 7.468
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

CWNU 1712 UCC
CWNU 1712 HUNT23

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.15, m-M=10.8, logAge=7.9
Hunt & Reffert (2023) AV50=0.653, diffAV50=1.168, MOD50=10.544, logAge50=8.685
Cavallo et al. (2024) AV50=0.58, dMod50=10.42, logAge50=8.75, [Fe/H]50=0.38
Hunt & Reffert (2024) MassJ=96.7087, MassTot=103.358
Hu & Soubiran (2025) MA22=-0.18, MA23f=-0.16, MZ23=-0.15, MK24=-0.19, MF24=-0.15

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Cluster region map