Berkeley 48

(NGC 6827; MWSC 3186; OCL 120; FSR 0152)

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C3
N_50
r_50
AA 141 1.0
Summary

Berkeley 48 is a rich, very dense object of very high C3 quality. It is located at a large distance from the Sun, below 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) 297.221 21.215 1.92 -5.07
Kharchenko et al. (2013) 297.213 21.215 1.4 -12.34
Kharchenko et al. (2016) 297.208 21.213
Cantat-Gaudin et al. (2018) 297.22 21.213 0.103 -2.418 -5.465
Bica et al. (2019) 297.227 21.22
Soubiran et al. (2018) 297.22 21.213 23.75
Cantat-Gaudin et al. (2020) 297.22 21.213 0.103 -2.418 -5.465
Dias et al. (2021) 297.22 21.214 0.095 -2.408 -5.465
Just et al. (2023) 297.208 21.213
Hunt & Reffert (2023) 297.222 21.214 0.124 -2.462 -5.456 -1.635
Cavallo et al. (2024) 297.225 21.207 0.119
Hunt & Reffert (2024) 297.222 21.214 0.124 -2.462 -5.456 -1.635
Almeida et al. (2025) 297.22 21.214
           
UCC 297.221 21.214 0.108 -2.453 -5.465 -8.165
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)=0.78, Dist=4550.0, Age=8.98
Kharchenko et al. (2013) E(B-V)=0.895, d=4192.0, logt=9.06
Kharchenko et al. (2016) E(B-V)=0.895, d=4192.0, logt=9.06
Cantat-Gaudin et al. (2018) dmode=7594.9
Soubiran et al. (2018) dmode=7594.9
Cantat-Gaudin et al. (2020) AVNN=1.98, DistPc=5735.0, AgeNN=9.11
Dias et al. (2021) Av=2.362, Dist=6471, logage=8.931, [Fe/H]=0.253
Just et al. (2023) logt=9.06, logmt=2.57
Hunt & Reffert (2023) AV50=3.178, diffAV50=2.329, MOD50=14.239, logAge50=8.354
Cavallo et al. (2024) AV50=3.42, dMod50=13.61, logAge50=8.52, [Fe/H]50=-0.7
Hunt & Reffert (2024) MassJ=3053.82, MassTot=3495.22
Almeida et al. (2025) AV=2.362, Dist=6471, logAge=8.931, MassRk=1632.5

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Cluster region map