Kronberger 92

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.27 0.94 0.5 0.33 1.0
C3
N_50
r_50
BB 27 6.6
Summary

Kronberger 92 is a poorly populated, very dense object of intermediate C3 quality. It is located at a relatively close distance from the Sun, above the mid-plane. It is poorly studied in the literature.

This object shares a large percentage of members with a later reported entry.

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Positions

Reference RA DEC Plx pmRA pmDE Rv
Bica et al. (2019) 83.831 44.166 – – – –
Hunt & Reffert (2023) 83.852 44.195 0.799 1.896 -2.541 -29.517
Cavallo et al. (2024) 83.873 44.199 0.797 – – –
Hunt & Reffert (2024) 83.852 44.195 0.799 1.896 -2.541 -29.517
           
UCC 83.9 44.172 0.801 1.934 -2.583 -28.682
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

Kronberger 92 UCC
Kronberger 92 HUNT23

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Fundamental parameters

Reference Values
Hunt & Reffert (2023) AV50=0.749, diffAV50=0.501, MOD50=10.375, logAge50=8.217
Cavallo et al. (2024) AV50=0.58, dMod50=10.44, logAge50=8.47, [Fe/H]50=0.4
Hunt & Reffert (2024) MassJ=74.3173, MassTot=116.851

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1158 88.9 83.85 44.17 0.8 1.93 -2.58 -30.59 0.01