CWNU 2452

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.4 0.83 0.38 0.33 1.0
C3
N_50
r_50
CB 40 2.1
Summary

CWNU 2452 is a poorly populated, dense object of low 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) 149.892 -58.718 0.205 -5.296 3.456 8.84
Hunt & Reffert (2023) 149.888 -58.713 0.194 -5.311 3.446 12.565
Cavallo et al. (2024) 149.873 -58.72 0.195 – – –
Hunt & Reffert (2024) 149.888 -58.713 0.194 -5.311 3.446 12.565
           
UCC 149.887 -58.714 0.196 -5.304 3.441 18.468
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

CWNU 2452 UCC
CWNU 2452 HUNT23

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Fundamental parameters

Reference Values
He et al. (2023) A0=2.1, m-M=13.0, logAge=8.75
Hunt & Reffert (2023) AV50=2.75, diffAV50=2.204, MOD50=13.431, logAge50=8.025
Cavallo et al. (2024) AV50=2.94, dMod50=13.08, logAge50=8.42, [Fe/H]50=-0.25
Hunt & Reffert (2024) MassJ=963.016, MassTot=997.038

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Cluster region map