CWNU 1714

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.35 0.89 0.75 0.42 1.0
C3
N_50
r_50
AB 35 1.6
Summary

CWNU 1714 is a poorly populated, dense object of high C3 quality. It is located at a large distance from the Sun, below the mid-plane. It was recently reported in the literature.

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Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2023) 100.596 -1.515 0.212 -0.072 0.534 –
Hunt & Reffert (2023) 100.595 -1.515 0.169 -0.121 0.548 87.248
Cavallo et al. (2024) 100.584 -1.52 0.164 – – –
Hunt & Reffert (2024) 100.595 -1.515 0.169 -0.121 0.548 87.248
Hu & Soubiran (2025) 100.584 -1.52 – – – –
           
UCC 100.59 -1.515 0.166 -0.12 0.544 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

CWNU 1714 UCC
CWNU 1714 HUNT23

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Fundamental parameters

Reference Values
He et al. (2023) A0=2.05, m-M=14.2, logAge=6.75
Hunt & Reffert (2023) AV50=1.828, diffAV50=2.188, MOD50=13.732, logAge50=8.349
Cavallo et al. (2024) AV50=1.53, dMod50=12.99, logAge50=8.8, [Fe/H]50=-0.14
Hunt & Reffert (2024) MassJ=1278.22, MassTot=1746.95
Hu & Soubiran (2025) MA22=-0.3, MA23f=-0.63, MK24=-0.43, MF24=-0.5

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Cluster region map