CWNU 1752

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.51 0.5 0.42 1.0
C3
N_50
r_50
BB 20 3.9
Summary

CWNU 1752 is a sparse, moderately dense object of intermediate C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It was recently reported in the literature.

Warning: contains less than 25 stars with P>0.5 estimated.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2023) 245.279 -52.638 0.41 -1.72 -2.352 -61.46
Hunt & Reffert (2023) 245.356 -52.673 0.412 -1.785 -2.385 -61.455
Cavallo et al. (2024) 245.303 -52.653 0.412 – – –
Hunt & Reffert (2024) 245.356 -52.673 0.412 -1.785 -2.385 -61.455
Hu & Soubiran (2025) 245.303 -52.653 – – – –
           
UCC 245.303 -52.649 0.407 -1.725 -2.366 -60.669
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

CWNU 1752 UCC
CWNU 1752 HUNT23

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.2, m-M=11.75, logAge=8.7
Hunt & Reffert (2023) AV50=1.023, diffAV50=0.806, MOD50=11.709, logAge50=8.513
Cavallo et al. (2024) AV50=1.57, dMod50=11.29, logAge50=8.73, [Fe/H]50=-0.49
Hunt & Reffert (2024) MassJ=177.822, MassTot=110.532
Hu & Soubiran (2025) MA22=-0.19, MA23f=-0.24, MZ23=0.19, MK24=-0.08, MF24=-0.01

Search coordinates in Bayestar19

Cluster region map