Berkeley 101

(FSR 0444; OCL 267; MWSC 3737)

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C3
N_50
r_50
AB 206 2.3
Summary

Berkeley 101 is a rich, very dense object of high C3 quality. It is located at a moderate distance from the Sun, above 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) 353.196 64.208 -2.05 -0.11
Froebrich et al. (2007) 353.208 64.213
Kharchenko et al. (2012) 353.188 64.205 -2.33 -0.44
Loktin & Popova (2017) 353.19 64.208 -2.05 -0.11
Cantat-Gaudin et al. (2018) 353.213 64.209 0.177 -1.899 -1.089
Bica et al. (2019) 353.195 64.196
Cantat-Gaudin et al. (2020) 353.213 64.209 0.177 -1.899 -1.089
Dias et al. (2021) 353.215 64.21 0.165 -1.869 -1.075
Hunt & Reffert (2023) 353.207 64.206 0.199 -1.86 -1.09 -66.733
Cavallo et al. (2024) 353.21 64.203 0.196
Hunt & Reffert (2024) 353.207 64.206 0.199 -1.86 -1.09 -66.733
Almeida et al. (2025) 353.215 64.21
Hu & Soubiran (2025) 353.21 64.203
           
UCC 353.203 64.205 0.202 -1.86 -1.093 -70.417
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)=0.98, Dist=2693.0, Age=8.75
Kharchenko et al. (2012) e_bv=0.949, distance=3000, log_age=8.86
Loktin & Popova (2017) E(B-V)=0.85, Dist=2844, logt=8.76
Cantat-Gaudin et al. (2018) dmode=4847.9
Cantat-Gaudin et al. (2020) AVNN=2.84, DistPc=4272.0, AgeNN=8.58
Dias et al. (2021) Av=3.009, Dist=4462, logage=8.642, [Fe/H]=-0.013
Hunt & Reffert (2023) AV50=3.334, diffAV50=1.424, MOD50=13.257, logAge50=8.337
Cavallo et al. (2024) AV50=3.06, dMod50=12.71, logAge50=8.86, [Fe/H]50=0.12
Hunt & Reffert (2024) MassJ=1892.69, MassTot=1892.69
Almeida et al. (2025) AV=3.009, Dist=4462, logAge=8.642, MassRk=728.7
Hu & Soubiran (2025) MA22=-0.41, MA23f=-0.44, MA23g=-0.27, MK24=-0.27, MF24=-0.47

Search coordinates in Bayestar19

Cluster region map