CWNU 1290

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.49 0.58 0.75 0.25 1.0
C3
N_50
r_50
AB 49 5.2
Summary

CWNU 1290 is a poorly populated, moderately dense object of high C3 quality. It is located at a moderate 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) 143.176 -55.816 0.368 -5.722 4.484 -1.39
Hunt & Reffert (2023) 143.155 -55.824 0.353 -5.703 4.502 –
Cavallo et al. (2024) 143.175 -55.829 0.356 – – –
Hunt & Reffert (2024) 143.155 -55.824 0.353 -5.703 4.502 –
           
UCC 143.161 -55.828 0.368 -5.687 4.481 0.811
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

CWNU 1290 UCC
CWNU 1290 HUNT23

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Fundamental parameters

Reference Values
He et al. (2023) A0=3.6, m-M=12.15, logAge=8.5
Hunt & Reffert (2023) AV50=2.668, diffAV50=2.297, MOD50=11.993, logAge50=8.711
Cavallo et al. (2024) AV50=3.51, dMod50=12.1, logAge50=8.52, [Fe/H]50=-0.11
Hunt & Reffert (2024) MassJ=369.180, MassTot=458.284

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Cluster region map