Berkeley 49

(FSR 0191; OCL 144)

UTI: UCC Trust Index C_N C_dens C_C3 C_lit C_dup 0.78 1.0 0.75 0.82 1.0
C3	N_50	r_50
AB	183	1.5

Summary

Berkeley 49 is a rich, very dense object of high C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It is well-studied in the literature.

This object shares a very small percentage of members with a later reported entry.

Search object in SciX | Simbad

Positions

Reference	RA	DEC	Plx	pmRA	pmDE	Rv
Dias et al. (2002)	299.875	34.642	–	-2.9	-3.3	–
Froebrich et al. (2007)	299.871	34.656	–	–	–	–
Kharchenko et al. (2012)	299.873	34.645	–	-2.9	-3.3	–
Loktin & Popova (2017)	299.865	34.652	–	-3.888	-3.645	–
Cantat-Gaudin et al. (2018)	299.872	34.643	0.286	-2.995	-6.095	–
Bica et al. (2019)	299.871	34.645	–	–	–	–
Soubiran et al. (2018)	299.872	34.643	–	–	–	-13.19
Cantat-Gaudin et al. (2020)	299.872	34.643	0.286	-2.995	-6.095	–
Hunt & Reffert (2023)	299.869	34.643	0.303	-3.024	-6.082	-20.271
Cavallo et al. (2024)	299.868	34.629	0.306	–	–	–
Hunt & Reffert (2024)	299.869	34.643	0.303	-3.024	-6.082	-20.271
UCC	299.867	34.643	0.297	-3.016	-6.085	-14.8

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)=1.18, Dist=2090.0, Age=8.9
Kharchenko et al. (2012)	e_bv=1.228, distance=2296, log_age=8.46
Loktin & Popova (2017)	E(B-V)=1.059, Dist=3781, logt=8.71
Cantat-Gaudin et al. (2018)	dmode=3175.0
Soubiran et al. (2018)	dmode=3175.0
Cantat-Gaudin et al. (2020)	AVNN=3.24, DistPc=3030.0, AgeNN=8.41
Hunt & Reffert (2023)	AV50=4.124, diffAV50=2.699, MOD50=12.355, logAge50=8.042
Cavallo et al. (2024)	AV50=4.22, dMod50=12.64, logAge50=7.8, [Fe/H]50=0.09
Hunt & Reffert (2024)	MassJ=2007.66, MassTot=2042.59

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Teutsch J2000.5+3432	1.1	300.14	34.54	0.24	-2.61	-6.31	-28.5	0.24