CWNU 132

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.74 1.0 1.0 0.25 1.0
C3
N_50
r_50
AA 98 5.1
Summary

CWNU 132 is a moderately populated, very dense object of very high C3 quality. It is located at a relatively close distance from the Sun, near 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. (2022) 276.503 -15.037 0.54 -1.4 -2.23 -2.9
Hunt & Reffert (2023) 276.49 -15.053 0.549 -1.399 -2.229 14.071
Cavallo et al. (2024) 276.51 -15.045 0.549 – – –
Hunt & Reffert (2024) 276.49 -15.053 0.549 -1.399 -2.229 14.071
           
UCC 276.509 -15.053 0.534 -1.403 -2.236 -3.141
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

CWNU 132 UCC
CWNU 132 HUNT23

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Fundamental parameters

Reference Values
He et al. (2022) AG=2.95, m-M=10.7, logAge=8.2, Z=0.006
Hunt & Reffert (2023) AV50=3.126, diffAV50=2.719, MOD50=11.174, logAge50=7.568
Cavallo et al. (2024) AV50=3.09, dMod50=10.65, logAge50=8.76, [Fe/H]50=-0.31
Hunt & Reffert (2024) MassJ=617.231, MassTot=617.231

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Cluster region map