Kronberger 4

(DSH J1945.1+2809; MWSC 3170)

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C3
N_50
r_50
AB 90 0.9
Summary

Kronberger 4 is a moderately populated, very dense object of high C3 quality. It is located at a large distance from the Sun, above the mid-plane. It is well-studied in the literature.

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Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 296.296 28.161 -2.8 -4.69
Kronberger et al. (2006) 296.298 28.161
Kharchenko et al. (2012) 296.288 28.167 -3.93 -5.63
Cantat-Gaudin et al. (2018) 296.297 28.16 0.119 -2.542 -4.836
Bica et al. (2019) 296.298 28.156
Cantat-Gaudin et al. (2020) 296.297 28.16 0.119 -2.542 -4.836
Dias et al. (2021) 296.297 28.16 0.126 -2.541 -4.817
Hunt & Reffert (2023) 296.292 28.163 0.13 -2.506 -4.899 -39.104
Cavallo et al. (2024) 296.295 28.16 0.13
Hunt & Reffert (2024) 296.292 28.163 0.13 -2.506 -4.899 -39.104
Almeida et al. (2025) 296.297 28.16
           
UCC 296.295 28.16 0.122 -2.528 -4.885 -43.274
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

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Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=0.56, Dist=7900.0
Kronberger et al. (2006) E(B-V)=0.56, Dist=7.9
Kharchenko et al. (2012) e_bv=0.437, distance=3731, log_age=9.1
Cantat-Gaudin et al. (2018) dmode=6765.2
Cantat-Gaudin et al. (2020) AVNN=2.19, DistPc=6984.0, AgeNN=8.83
Dias et al. (2021) Av=2.363, Dist=7318, logage=8.923, [Fe/H]=0.278
Hunt & Reffert (2023) AV50=3.104, diffAV50=2.214, MOD50=14.093, logAge50=7.711
Cavallo et al. (2024) AV50=3.31, dMod50=13.6, logAge50=8.25, [Fe/H]50=-0.32
Hunt & Reffert (2024) MassJ=792.651, MassTot=977.881
Almeida et al. (2025) AV=2.363, Dist=7318, logAge=8.923, MassRk=1110.8

Search coordinates in Bayestar19

Cluster region map