Berkeley 36

(OCL 577; FSR 1214; MWSC 1156)

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C3
N_50
r_50
AB 1179 3.9
Summary

Berkeley 36 is a very rich, very dense object of high C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is well-studied in the literature.

This object shares a very small percentage of members with 2 later reported entries.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 109.1 -13.193 -1.15 2.32
Kharchenko et al. (2012) 109.083 -13.178 3.31 2.63
Cantat-Gaudin et al. (2018) 109.105 -13.196 0.206 -1.725 0.86
Bica et al. (2019) 109.095 -13.193
Soubiran et al. (2018) 109.105 -13.196 63.54
Cantat-Gaudin et al. (2020) 109.105 -13.196 0.206 -1.725 0.86
Dias et al. (2021) 109.104 -13.201 0.182 -1.745 0.874 63.526
Hunt & Reffert (2023) 109.1 -13.193 0.212 -1.693 0.958 62.662
Cavallo et al. (2024) 109.087 -13.201 0.215
Hunt & Reffert (2024) 109.1 -13.193 0.212 -1.693 0.958 62.662
Almeida et al. (2025) 109.104 -13.201
           
UCC 109.097 -13.197 0.226 -1.684 0.957 62.801
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

Explore data in Colab

Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=0.4, Dist=6140.0, Age=9.5
Kharchenko et al. (2012) e_bv=0.583, distance=5041, log_age=9.4
Cantat-Gaudin et al. (2018) dmode=4253.5
Soubiran et al. (2018) dmode=4253.5
Cantat-Gaudin et al. (2020) AVNN=1.42, DistPc=4360.0, AgeNN=9.83
Dias et al. (2021) Av=1.8, Dist=4978, logage=9.533, [Fe/H]=-0.03
Hunt & Reffert (2023) AV50=1.946, diffAV50=2.382, MOD50=12.944, logAge50=9.018
Cavallo et al. (2024) AV50=1.63, dMod50=12.76, logAge50=9.26, [Fe/H]50=-0.03
Hunt & Reffert (2024) MassJ=2690.48, MassTot=2816.07
Almeida et al. (2025) AV=1.8, Dist=4978, logAge=9.533, MassRk=3807.6

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0387 2.1 109.09 -13.19 0.23 -1.7 0.96 62.55 0.0
OC 0388 2.1 109.12 -13.18 0.16 -1.75 0.98 60.37 0.0