Berkeley 20

(OCL 497; MWSC 572)

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C3
N_50
r_50
AA 224 1.3
Summary

Berkeley 20 is a rich, very dense object of very high C3 quality. It is located at a very large distance from the Sun, well below the mid-plane. It is very well-studied in the literature.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 83.154 0.188 1.51 -4.11 70.0
Chen et al. (2003) 83.248 0.21
Kharchenko et al. (2012) 83.154 0.183 -1.62 -4.26
Loktin & Popova (2017) 83.16 -0.188 1.51 -4.11 75.7
Cantat-Gaudin et al. (2018) 83.152 0.185 0.04 0.808 -0.244
Bica et al. (2019) 83.16 0.184
Donor et al. (2020) 83.154 0.183 1.04 -0.16 78.8
Cantat-Gaudin et al. (2020) 83.152 0.185 0.04 0.808 -0.244
Rain et al. (2021) 83.152 0.185 0.04 0.808 -0.244
Jaehnig et al. (2021) 83.155 0.189 0.045 0.82 -0.259
Hunt & Reffert (2023) 83.154 0.188 0.094 0.827 -0.246 78.888
Cavallo et al. (2024) 83.142 0.177 0.116
Hunt & Reffert (2024) 83.154 0.188 0.094 0.827 -0.246 78.888
           
UCC 83.153 0.186 0.1 0.869 -0.231 79.133
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

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Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=0.12, Dist=8400.0, Age=9.78, [Fe/H]=-0.3
Chen et al. (2003) E(B-V)=0.12, HDis=8400, Age=6.02, [Fe/H]_1=-0.75
Kharchenko et al. (2012) e_bv=0.121, distance=8399, log_age=9.78, metallicity=-0.61
Loktin & Popova (2017) E(B-V)=1.5, Dist=8802, logt=9.729
Cantat-Gaudin et al. (2018) dmode=14402.1
Donor et al. (2020) Fe/H=-0.4
Cantat-Gaudin et al. (2020) AVNN=0.37, DistPc=8728.0, AgeNN=9.68
Rain et al. (2021) E(B-V)=0.12, Dist=14402.1, log(Age)=9.78, NBSS=6
Jaehnig et al. (2021) dmode=14.228
Hunt & Reffert (2023) AV50=0.461, diffAV50=1.689, MOD50=14.514, logAge50=9.265
Cavallo et al. (2024) AV50=1.35, dMod50=13.02, logAge50=9.79, [Fe/H]50=-0.72
Hunt & Reffert (2024) MassJ=833.904, MassTot=1145.08

Search coordinates in Bayestar19

Cluster region map