Berkeley 47

(MWSC 3126; OCL 109)

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C3
N_50
r_50
AA 126 2.4
Summary

Berkeley 47 is a rich, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is well-studied in the literature.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 292.15 17.368 0.45 0.88
Kharchenko et al. (2013) 292.117 17.36 -1.49 -4.51
Kharchenko et al. (2016) 292.112 17.357
Loktin & Popova (2017) 292.125 17.366 -0.931 -4.106
Cantat-Gaudin et al. (2018) 292.127 17.362 0.402 -1.894 -5.444
Bica et al. (2019) 292.123 17.358
Cantat-Gaudin et al. (2020) 292.127 17.362 0.402 -1.894 -5.444
Dias et al. (2021) 292.129 17.364 0.396 -1.868 -5.433
Just et al. (2023) 292.112 17.357
Hunt & Reffert (2023) 292.126 17.361 0.403 -1.94 -5.466 94.682
Cavallo et al. (2024) 292.134 17.355 0.403
Celli et al. (2024) 292.127 17.362
Hunt & Reffert (2024) 292.126 17.361 0.403 -1.94 -5.466 94.682
Almeida et al. (2025) 292.129 17.364
           
UCC 292.131 17.358 0.403 -1.939 -5.452 23.165
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)=1.5, Dist=1070.0, Age=8.7
Kharchenko et al. (2013) E(B-V)=1.166, d=1462.0, logt=7.97
Kharchenko et al. (2016) E(B-V)=1.166, d=1462.0, logt=7.97
Loktin & Popova (2017) E(B-V)=0.973, Dist=2534, logt=8.1
Cantat-Gaudin et al. (2018) dmode=2323.0
Cantat-Gaudin et al. (2020) AVNN=4.02, DistPc=2437.0, AgeNN=7.34
Dias et al. (2021) Av=3.63, Dist=1974, logage=7.148, [Fe/H]=0.137
Just et al. (2023) logt=7.97, logmt=2.093
Hunt & Reffert (2023) AV50=4.623, diffAV50=1.437, MOD50=11.87, logAge50=7.029
Cavallo et al. (2024) AV50=4.43, dMod50=11.4, logAge50=7.23, [Fe/H]50=-0.32
Celli et al. (2024) Age=21.9, Mc=631.2
Hunt & Reffert (2024) MassJ=1595.10, MassTot=1606.94
Almeida et al. (2025) AV=3.63, Dist=1974, logAge=7.148, MassRk=403.4

Search coordinates in Bayestar19

Cluster region map