King 26

(OCL 108; MWSC 3128)

UTI: UCC Trust Index C_N C_dens C_C3 C_lit C_dup 0.75 1.0 1.0 0.86 1.0
C3	N_50	r_50
AA	102	2.2

Summary

King 26 is a rich, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is well-studied in the literature.

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Positions

Reference	RA	DEC	Plx	pmRA	pmDE	Rv
Dias et al. (2002)	292.254	14.867	–	0.21	-2.55	–
Kharchenko et al. (2012)	292.24	14.873	–	-1.55	-7.66	–
Loktin & Popova (2017)	292.245	14.867	–	-1.186	-6.445	–
Cantat-Gaudin et al. (2018)	292.237	14.882	0.414	-2.344	-4.935	–
Bica et al. (2019)	292.242	14.871	–	–	–	–
Soubiran et al. (2018)	292.237	14.882	–	–	–	25.01
Cantat-Gaudin et al. (2020)	292.237	14.882	0.414	-2.344	-4.935	–
Dias et al. (2021)	292.233	14.887	0.412	-2.329	-4.907	–
Hunt & Reffert (2023)	292.235	14.881	0.411	-2.376	-4.969	24.707
Cavallo et al. (2024)	292.242	14.891	0.412	–	–	–
Hunt & Reffert (2024)	292.235	14.881	0.411	-2.376	-4.969	24.707
Almeida et al. (2025)	292.233	14.887	–	–	–	–
UCC	292.237	14.881	0.412	-2.37	-4.985	24.799

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)=1.27, Dist=2600.0, Age=8.64
Kharchenko et al. (2012)	e_bv=1.02, distance=2537, log_age=8.68
Loktin & Popova (2017)	E(B-V)=0.598, Dist=2410, logt=8.86
Cantat-Gaudin et al. (2018)	dmode=2256.2
Soubiran et al. (2018)	dmode=2256.2
Cantat-Gaudin et al. (2020)	AVNN=2.71, DistPc=2281.0, AgeNN=8.37
Dias et al. (2021)	Av=2.988, Dist=2169, logage=7.686, [Fe/H]=0.318
Hunt & Reffert (2023)	AV50=3.376, diffAV50=1.512, MOD50=11.744, logAge50=8.084
Cavallo et al. (2024)	AV50=3.3, dMod50=11.93, logAge50=8.09, [Fe/H]50=0.49
Hunt & Reffert (2024)	MassJ=1044.24, MassTot=1153.27
Almeida et al. (2025)	AV=2.988, Dist=2169, logAge=7.686, MassRk=486.1

Search coordinates in Bayestar19

Cluster region map