Berkeley 59

UTI: UCC Trust Index C_N C_dens C_C3 C_lit C_dup 1.0 1.0 0.75 0.86 1.0
C3	N_50	r_50
AB	530	5.4

Summary

Berkeley 59 is a very rich, very dense object of high C3 quality. It is located at a relatively close 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)	0.558	67.417	–	-2.11	-1.2	-5.17
Piskunov et al. (2008)	0.554	67.42	–	–	–	–
Kharchenko et al. (2012)	0.559	67.425	–	-3.2	-1.11	–
Loktin & Popova (2017)	0.555	67.417	–	-0.752	-0.589	-12.5
Cantat-Gaudin et al. (2018)	0.57	67.441	0.916	-1.616	-1.764	–
Cantat-Gaudin et al. (2020)	0.57	67.441	0.916	-1.616	-1.764	–
Dias et al. (2021)	8.654	67.464	0.893	-1.597	-1.841	–
He et al. (2022)	0.522	67.581	0.96	-1.623	-1.635	–
Hunt & Reffert (2023)	0.57	67.429	0.96	-1.61	-1.699	-3.264
Cavallo et al. (2024)	0.608	67.648	0.959	–	–	–
Celli et al. (2024)	0.57	67.441	–	–	–	–
Hunt & Reffert (2024)	0.57	67.429	0.96	-1.61	-1.699	-3.264
UCC	0.575	67.447	0.95	-1.634	-1.845	-14.086

Galactocentric position

How are the galactocentric plots generated?

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Estimated members

1 2 3

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Fundamental parameters

Reference	Values
Dias et al. (2002)	E(B-V)=1.241, Dist=1000.0, Age=6.1
Piskunov et al. (2008)	E(B-V)=1.22, Dist=1000, logt=6.8, logMA=2.221
Kharchenko et al. (2012)	e_bv=1.241, distance=1000, log_age=6.1
Loktin & Popova (2017)	E(B-V)=0.953, Dist=1519, logt=6.98
Cantat-Gaudin et al. (2018)	dmode=1058.1
Dias et al. (2021)	Av=3.82, Dist=1026, logage=6.8, [Fe/H]=0.001
He et al. (2022)	A0=4.95, logAge=6.6
Hunt & Reffert (2023)	AV50=3.805, diffAV50=3.009, MOD50=10.049, logAge50=6.7
Cavallo et al. (2024)	AV50=3.85, dMod50=10.33, logAge50=6.7, [Fe/H]50=0.01
Celli et al. (2024)	Age=1.3, Mc=1323.8
Hunt & Reffert (2024)	MassJ=4317.11, MassTot=4378.79

Search coordinates in Bayestar19

Cluster region map