Berkeley 61

(OCL 308; FSR 0514; MWSC 75)

Click to load Aladin Lite
C3
N_50
r_50
AC 113 3.1
Summary

Berkeley 61 is a rich, very dense object of intermediate C3 quality. It is located at a moderate distance from the Sun, above 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) 12.125 67.2 -7.26 0.35
Kharchenko et al. (2012) 12.079 67.193 -1.95 0.98
Loktin & Popova (2017) 12.075 67.2 -3.661 1.21
Cantat-Gaudin et al. (2018) 12.04 67.199 0.309 -2.505 -0.014
Bica et al. (2019) 12.057 67.19
Bossini et al. (2019) 12.04 67.199
Cantat-Gaudin et al. (2020) 12.04 67.199 0.309 -2.505 -0.014
Dias et al. (2021) 12.049 67.203 0.32 -2.486 -0.028
Hunt & Reffert (2023) 12.043 67.198 0.288 -2.496 -0.14 -54.991
Cavallo et al. (2024) 12.034 67.202 0.292
Hunt & Reffert (2024) 12.043 67.198 0.288 -2.496 -0.14 -54.991
Almeida et al. (2025) 12.049 67.203
           
UCC 12.032 67.201 0.291 -2.508 -0.113 -59.329
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)=0.69, Dist=3798.0, Age=8.25
Kharchenko et al. (2012) e_bv=1.041, distance=2153, log_age=8.985
Loktin & Popova (2017) E(B-V)=0.612, Dist=2498, logt=7.6
Cantat-Gaudin et al. (2018) dmode=2958.0
Bossini et al. (2019) AV=2.135, Dist=12.545, logA=8.165, Fe/H=0.0
Cantat-Gaudin et al. (2020) AVNN=2.07, DistPc=2922.0, AgeNN=8.26
Dias et al. (2021) Av=2.456, Dist=2638, logage=8.294, [Fe/H]=-0.11
Hunt & Reffert (2023) AV50=2.55, diffAV50=1.228, MOD50=12.504, logAge50=8.197
Cavallo et al. (2024) AV50=2.86, dMod50=12.88, logAge50=7.35, [Fe/H]50=-0.33
Hunt & Reffert (2024) MassJ=605.059, MassTot=606.033
Almeida et al. (2025) AV=2.456, Dist=2638, logAge=8.294, MassRk=309.1

Search coordinates in Bayestar19

Cluster region map