Berkeley 14A

(MWSC 449)

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C3
N_50
r_50
AC 35 11.1
Summary

Berkeley 14A is a poorly populated, moderately dense object of intermediate C3 quality. It is located at a relatively close distance from the Sun, near the mid-plane. It is well-studied in the literature.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Kharchenko et al. (2005) 75.1 43.48 -0.73 -2.94 4.82
Piskunov et al. (2007) 75.092 43.481
Kharchenko et al. (2007) 75.04 43.47 0.74 4.82
Piskunov et al. (2008) 75.092 43.481
Cantat-Gaudin et al. (2018) 75.278 43.429 0.882 -0.225 -2.741
Bica et al. (2019) 75.156 43.568
Cantat-Gaudin et al. (2020) 75.278 43.429 0.882 -0.225 -2.741
He et al. (2022) 75.108 43.611 0.88 -0.369 -2.802
Hunt & Reffert (2023) 75.046 43.679 0.889 -0.324 -2.785 -12.268
Cavallo et al. (2024) 75.137 43.564 0.887
Celli et al. (2024) 75.278 43.429
Hunt & Reffert (2024) 75.046 43.679 0.889 -0.324 -2.785 -12.268
Zhang et al. (2024) 75.046 43.679
           
UCC 75.117 43.58 0.88 -0.317 -2.772 0.193
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
Kharchenko et al. (2005) E(B-V)=0.23, Dist=1100, logt=6.97
Piskunov et al. (2007) E(B-V)=0.23, Dist=1100, logt=6.97, logM=3.467
Piskunov et al. (2008) E(B-V)=0.23, Dist=1100, logt=6.97, logM=3.941, logMA=3.874
Cantat-Gaudin et al. (2018) dmode=1097.1
He et al. (2022) A0=1.0, logAge=7.4
Hunt & Reffert (2023) AV50=0.562, diffAV50=0.858, MOD50=10.16, logAge50=7.566
Cavallo et al. (2024) AV50=1.17, dMod50=10.25, logAge50=7.23, [Fe/H]50=-0.2
Celli et al. (2024) Age=9.3, Mc=97.0
Hunt & Reffert (2024) MassJ=100.561, MassTot=106.016
Zhang et al. (2024) [Fe/H]ANN=-0.3673, [Fe/H]MCMC=-0.3660

Search coordinates in Bayestar19

Cluster region map