CWNU 52

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.13 0.5 0.31 1.0
C3
N_50
r_50
BB 24 33.5
Summary

CWNU 52 is a sparse, very loose object of intermediate C3 quality. It is located at a close 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. (2022) 72.206 26.227 1.62 -1.81 -2.34 –
Hunt & Reffert (2023) 72.339 26.185 1.616 -1.728 -2.281 -7.845
Cavallo et al. (2024) 72.37 26.201 1.616 – – –
Hunt & Reffert (2024) 72.339 26.185 1.616 -1.728 -2.281 -7.845
Zhang et al. (2024) 72.339 26.185 – – – –
           
UCC 72.238 26.389 1.625 -1.812 -2.303 -5.324
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

CWNU 52 UCC
CWNU 52 HUNT23

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Fundamental parameters

Reference Values
He et al. (2022) AG=2.45, m-M=8.85, logAge=7.7, Z=0.006
Hunt & Reffert (2023) AV50=1.987, diffAV50=2.461, MOD50=8.823, logAge50=7.744
Cavallo et al. (2024) AV50=2.25, dMod50=9.07, logAge50=7.74, [Fe/H]50=0.4
Hunt & Reffert (2024) MassJ=97.1886, MassTot=215.953
Zhang et al. (2024) [Fe/H]ANN=-0.1621, [Fe/H]MCMC=-0.1411

Search coordinates in Bayestar19

Cluster region map