Berkeley 100

(MWSC 3727; OCL 264)

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C3
N_50
r_50
AB 109 1.8
Summary

Berkeley 100 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 moderately studied in the literature.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 351.492 63.78 -1.25 -2.58
Kharchenko et al. (2012) 351.477 63.778 -1.25 -2.58
Kharchenko et al. (2013) 351.477 63.778 -1.25 -2.58
Kharchenko et al. (2016) 351.468 63.775
Bica et al. (2019) 351.491 63.782
Cantat-Gaudin et al. (2020) 351.485 63.781 0.123 -3.372 -1.557
Just et al. (2023) 351.468 63.775
Hunt & Reffert (2023) 351.489 63.78 0.173 -3.265 -1.459 -45.808
Cavallo et al. (2024) 351.502 63.784 0.172
Hunt & Reffert (2024) 351.489 63.78 0.173 -3.265 -1.459 -45.808
           
UCC 351.484 63.779 0.165 -3.267 -1.475 -65.069
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)=1.0, Dist=3775.0, Age=8.05
Kharchenko et al. (2012) E(B-V)=1.21, d=2700.0, logt=7.432
Kharchenko et al. (2013) E(B-V)=1.21, d=2700.0, logt=7.432
Kharchenko et al. (2016) E(B-V)=1.21, d=2700.0, logt=7.432
Cantat-Gaudin et al. (2020) AVNN=2.48, DistPc=6084.0, AgeNN=9.09
Just et al. (2023) logt=7.432, logmt=1.277
Hunt & Reffert (2023) AV50=3.102, diffAV50=2.147, MOD50=13.426, logAge50=8.353
Cavallo et al. (2024) AV50=3.6, dMod50=13.68, logAge50=8.45, [Fe/H]50=-0.35
Hunt & Reffert (2024) MassJ=1051.91, MassTot=1192.23

Search coordinates in Bayestar19

Cluster region map