CWNU 1592

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.37 1.0 0.12 0.33 0.92
C3
N_50
r_50
DC 37 2.6
Summary

CWNU 1592 is a poorly populated, very dense object of very low C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It was recently reported in the literature.

This is very likely a unique object, which shares a very small percentage of members with at least one previously reported entry.

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Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2023) 112.661 -23.157 0.325 -1.721 1.727 84.98
Hunt & Reffert (2023) 112.682 -23.148 0.328 -1.768 1.712 –
Cavallo et al. (2024) 112.675 -23.153 0.328 – – –
Hunt & Reffert (2024) 112.682 -23.148 0.328 -1.768 1.712 –
           
UCC 112.668 -23.148 0.323 -1.76 1.723 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

CWNU 1592 UCC
CWNU 1592 HUNT23

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Fundamental parameters

Reference Values
He et al. (2023) A0=2.2, m-M=12.25, logAge=8.7
Hunt & Reffert (2023) AV50=1.905, diffAV50=1.333, MOD50=12.378, logAge50=7.712
Cavallo et al. (2024) AV50=2.33, dMod50=12.55, logAge50=7.77, [Fe/H]50=0.0
Hunt & Reffert (2024) MassJ=252.268, MassTot=252.268

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Ruprecht 23 8.1 112.66 -23.38 0.34 -2.06 1.61 59.89 0.91