Berkeley 5

(MWSC 142; OCL 331)

UTI: UCC Trust Index C_N C_dens C_C3 C_lit C_dup 0.78 1.0 0.75 0.5 1.0
C3	N_50	r_50
AB	172	1.2

Summary

Berkeley 5 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)	26.95	62.933	–	0.11	-2.78	–
Kharchenko et al. (2012)	26.925	62.933	–	0.11	-2.78	–
Kharchenko et al. (2013)	26.925	62.933	–	0.11	-2.78	–
Kharchenko et al. (2016)	26.913	62.93	–	–	–	–
Cantat-Gaudin et al. (2018)	26.928	62.935	0.088	-1.61	0.764	–
Bica et al. (2019)	26.928	62.946	–	–	–	–
Cantat-Gaudin et al. (2020)	26.928	62.935	0.088	-1.61	0.764	–
Just et al. (2023)	26.913	62.93	–	–	–	–
UCC	26.931	62.941	0.13	-1.599	0.677	-98.399

Galactocentric position

How are the galactocentric plots generated?

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Estimated members

1 2

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Fundamental parameters

Reference	Values
Dias et al. (2002)	E(B-V)=1.3, Dist=6200.0, Age=8.9
Kharchenko et al. (2012)	E(B-V)=1.399, d=6000.0, logt=8.83
Kharchenko et al. (2013)	E(B-V)=1.399, d=6000.0, logt=8.83
Kharchenko et al. (2016)	E(B-V)=1.399, d=6000.0, logt=8.83
Cantat-Gaudin et al. (2018)	dmode=8555.1
Cantat-Gaudin et al. (2020)	AVNN=3.46, DistPc=7079.0, AgeNN=9.06
Just et al. (2023)	logt=8.83, logmt=2.45

Search coordinates in Bayestar19

Cluster region map