Berkeley 35

(FSR 1075; OCL 541; MWSC 1129; MWSC 1130)

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C3
N_50
r_50
AB 259 3.3
Summary

Berkeley 35 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 very well-studied in the literature.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 107.483 2.734 -3.29 3.34
Froebrich et al. (2007) 107.5 2.716
Kharchenko et al. (2012) 107.484 2.733 -7.78 2.28
Loktin & Popova (2017) 107.49 2.734 -7.384 -0.022
Cantat-Gaudin et al. (2018) 107.491 2.734 0.16 -0.58 -0.235
Bica et al. (2019) 107.482 2.736
Soubiran et al. (2018) 107.491 2.734 101.46
Cantat-Gaudin et al. (2020) 107.491 2.734 0.16 -0.58 -0.235
Dias et al. (2021) 107.489 2.734 0.162 -0.587 -0.235
Hunt & Reffert (2023) 107.48 2.731 0.177 -0.611 -0.255 84.127
Cavallo et al. (2024) 107.482 2.729 0.176
Hunt & Reffert (2024) 107.48 2.731 0.177 -0.611 -0.255 84.127
Almeida et al. (2025) 107.489 2.734
Hu & Soubiran (2025) 107.482 2.729
           
UCC 107.486 2.733 0.181 -0.607 -0.251 81.2
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)=0.47, Dist=4390.0, Age=8.95, [Fe/H]=-0.13
Kharchenko et al. (2012) e_bv=0.0, distance=5012, log_age=9.065
Loktin & Popova (2017) E(B-V)=0.0, Dist=3370, logt=9.14
Cantat-Gaudin et al. (2018) dmode=5281.1
Soubiran et al. (2018) dmode=5281.1
Cantat-Gaudin et al. (2020) AVNN=0.43, DistPc=4745.0, AgeNN=9.07
Dias et al. (2021) Av=0.65, Dist=4639, logage=9.053, [Fe/H]=-0.301
Hunt & Reffert (2023) AV50=0.231, diffAV50=0.728, MOD50=13.871, logAge50=8.918
Cavallo et al. (2024) AV50=0.41, dMod50=12.56, logAge50=9.28, [Fe/H]50=-0.39
Hunt & Reffert (2024) MassJ=1399.51, MassTot=1418.60
Almeida et al. (2025) AV=0.65, Dist=4639, logAge=9.053, MassRk=263.7
Hu & Soubiran (2025) MA22=-0.32, MA23f=-0.56, MA23g=-0.38, MZ23=-0.4, MK24=-0.34, MF24=-0.42

Search coordinates in Bayestar19

Cluster region map