Berkeley 34

(Biurakan 13; OCL 543; MWSC 1058)

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C3
N_50
r_50
AB 240 1.6
Summary

Berkeley 34 is a rich, very dense object of high C3 quality. It is located at a large distance from the Sun, above the mid-plane. It is moderately studied in the literature.

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Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 105.096 -0.232 -2.68 -2.16
Kharchenko et al. (2012) 105.09 -0.235 -2.68 -2.16
Cantat-Gaudin et al. (2018) 105.097 -0.239 0.097 -1.336 0.175
Bica et al. (2019) 105.093 -0.235
Cantat-Gaudin et al. (2020) 105.097 -0.239 0.097 -1.336 0.175
Hunt & Reffert (2023) 105.094 -0.237 0.158 -1.292 0.176 73.329
Cavallo et al. (2024) 105.1 -0.235 0.148
Hunt & Reffert (2024) 105.094 -0.237 0.158 -1.292 0.176 73.329
           
UCC 105.097 -0.236 0.169 -1.347 0.183 83.132
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)=0.45, Dist=7280.0, Age=9.45
Kharchenko et al. (2012) e_bv=0.45, distance=7279, log_age=9.45
Cantat-Gaudin et al. (2018) dmode=7915.3
Cantat-Gaudin et al. (2020) AVNN=1.64, DistPc=7609.0, AgeNN=9.38
Hunt & Reffert (2023) AV50=1.383, diffAV50=2.397, MOD50=13.547, logAge50=8.285
Cavallo et al. (2024) AV50=1.8, dMod50=13.41, logAge50=8.74, [Fe/H]50=-0.22
Hunt & Reffert (2024) MassJ=463.455, MassTot=382.987

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Cluster region map