CWNU 1715

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.33 1.0 0.75 0.33 1.0
C3
N_50
r_50
BA 33 1.2
Summary

CWNU 1715 is a poorly populated, very dense object of high C3 quality. It is located at a moderate distance from the Sun, well above 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) 50.936 67.349 0.22 0.138 -0.218 –
Hunt & Reffert (2023) 50.936 67.348 0.186 0.102 -0.194 -46.705
Cavallo et al. (2024) 50.964 67.344 0.189 – – –
Hunt & Reffert (2024) 50.936 67.348 0.186 0.102 -0.194 -46.705
           
UCC 50.933 67.348 0.205 0.135 -0.223 -46.71
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

CWNU 1715 UCC
CWNU 1715 HUNT23

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Fundamental parameters

Reference Values
He et al. (2023) A0=3.2, m-M=13.5, logAge=8.65
Hunt & Reffert (2023) AV50=2.699, diffAV50=1.722, MOD50=13.289, logAge50=8.69
Cavallo et al. (2024) AV50=3.28, dMod50=13.63, logAge50=8.37, [Fe/H]50=-0.02
Hunt & Reffert (2024) MassJ=839.146, MassTot=933.383

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Cluster region map