King 14

(MWSC 57; Alter 1; OCL 297)

0.92 UTI

0.84

C_N

1.0

C_dens

0.75

C_C3

1.0

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 349

Radius (P>50% members) 5.1 [arcmin]

C_N 0.84 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 1.0 Very well-studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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King 14 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is very well-studied in the literature.

Relatively close Moderate extinction Near-solar metallicity Young

Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit.

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for King 14 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	7.988	63.175	0.393	-3.243	-1.054	-74.176
Li et al.	2025	7.987	63.163	0.402	-3.267	-0.985	–
Almeida et al.	2025	8.004	63.164	–	–	–	–
Hunt & Reffert	2024	7.986	63.171	0.393	-3.257	-1.085	–
Cavallo et al.	2024	7.994	63.173	0.392	–	–	–
Hunt & Reffert	2023	7.986	63.171	0.393	-3.257	-1.085	–
Almeida et al.	2023	8.007	63.167	–	–	–	–
Just et al.	2023	8.004	63.177	–	–	–	–
Jaehnig et al.	2021	7.973	63.157	0.436	-3.264	-1.025	–
Rain et al.	2021	7.987	63.163	0.402	-3.267	-0.985	–
Dias et al.	2021	8.004	63.164	0.4	-3.268	-0.995	–
Cantat-Gaudin et al.	2020	7.987	63.163	0.402	-3.267	-0.985	–
Sánchez et al.	2020	8.012	63.156	–	-3.246	-1.074	–
Cantat-Gaudin & Anders	2020	7.987	63.163	0.402	-3.267	-0.985	–
Bica et al.	2019	7.978	63.158	–	–	–	–
Cantat-Gaudin et al.	2018	7.987	63.163	0.402	-3.267	-0.985	–
Loktin & Popova	2017	8.01	63.156	–	-1.678	-2.675	–
Kharchenko et al.	2016	8.004	63.177	–	–	–	–
Dias et al.	2014	8.012	63.156	–	-2.25	0.73	–
Kharchenko et al.	2013	8.014	63.181	–	-3.75	-1.55	–
Kharchenko et al.	2012	8.014	63.181	–	-3.77	-1.53	–
van den Bergh	2006	7.975	63.167	–	–	–	–
Dias et al.	2002	8.012	63.156	–	-2.25	0.73	–

💡 Note: The UCC values are estimated from its identified members.

Reference	Year	Dist [kpc]	Av [mag]	DAv [mag]	Age [Myr]	[Fe/H] [dex]	Mass [Msun]	Bfr	BSS
Li et al.	2025	2.29	1.46	–	72	0.059	–	–	–
Almeida et al.	2025	2.21	1.59	–	46	–	592	–	–
Hunt & Reffert	2024	–	–	–	–	–	855*	–	–
Cavallo et al.	2024	2.26	1.72	–	48	-0.080	–	–	–
Hunt & Reffert	2023	2.38	1.53	1.09	48	–	–	–	–
Almeida et al.	2023	2.23	1.68	–	30	-0.019	870*	0.55	–
Just et al.	2023	–	–	–	50	–	317	–	–
Jaehnig et al.	2021	2.28*	–	–	–	–	–	–	–
Rain et al.	2021	2.32	1.05	–	79	–	–	–	0
Dias et al.	2021	2.21	1.59	–	46	-0.048	–	–	–
Cantat-Gaudin et al.	2020	2.42	1.30	–	145	–	–	–	–
Cantat-Gaudin & Anders	2020	2.32	–	–	–	–	–	–	–
Cantat-Gaudin et al.	2018	2.32	–	–	–	–	–	–	–
Loktin & Popova	2017	2.57	1.28	–	85	–	–	–	–
Kharchenko et al.	2016	2.60	1.86	–	50	–	–	–	–
Kharchenko et al.	2013	2.60	1.86	–	50	–	–	–	–
Kharchenko et al.	2012	2.60	1.86	–	50	–	–	–	–
van den Bergh	2006	2.59	1.27	–	83	–	–	–	–
Dias et al.	2002	2.96	1.05	–	79	–	–	–	–

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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