Berkeley 103

(OCL 266; MWSC 3755)

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C3
N_50
r_50
AA 119 1.0
Summary

Berkeley 103 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 moderately studied in the literature.

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Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 356.3 59.3 1.02 -3.93
Kharchenko et al. (2012) 356.317 59.3 1.02 -3.93
Cantat-Gaudin et al. (2018) 356.303 59.297 0.093 -1.348 -0.861
Bica et al. (2019) 356.305 59.301
Cantat-Gaudin et al. (2020) 356.303 59.297 0.093 -1.348 -0.861
Hunt & Reffert (2023) 356.303 59.299 0.144 -1.429 -0.954 -83.416
Cavallo et al. (2024) 356.302 59.297 0.155
Hunt & Reffert (2024) 356.303 59.299 0.144 -1.429 -0.954 -83.416
           
UCC 356.303 59.297 0.13 -1.367 -0.928 -80.711
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)=0.87, Dist=7379.0, Age=8.95, [Fe/H]=-0.38
Kharchenko et al. (2012) e_bv=0.999, distance=1800, log_age=8.7, metallicity=-0.38
Cantat-Gaudin et al. (2018) dmode=8173.4
Cantat-Gaudin et al. (2020) AVNN=2.4, DistPc=6060.0, AgeNN=9.04
Hunt & Reffert (2023) AV50=3.079, diffAV50=2.161, MOD50=13.88, logAge50=8.636
Cavallo et al. (2024) AV50=3.26, dMod50=14.1, logAge50=8.52, [Fe/H]50=-0.4
Hunt & Reffert (2024) MassJ=928.996, MassTot=1182.03

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Cluster region map