Czernik 13

(MWSC 227; OCL 356)

0.91 UTI

0.79

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%) 217

Radius (P>50% members) 3.2 [arcmin]

C_N 0.79 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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Czernik 13 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is very well-studied in the literature.

Distant Moderate extinction Near-solar metallicity Very young

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

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for Czernik 13 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	–	41.097	62.325	0.301	0.57	-0.281	-55.736
Li et al.	2025	41.106	62.327	0.293	0.585	-0.208	–
Almeida et al.	2025	41.112	62.329	–	–	–	–
Hunt & Reffert	2024	41.116	62.321	0.306	0.568	-0.294	-55.735
Cavallo et al.	2024	41.083	62.322	0.301	–	–	–
Hunt & Reffert	2023	41.116	62.321	0.306	0.568	-0.294	-55.735
Almeida et al.	2023	41.105	62.329	–	–	–	–
Just et al.	2023	41.102	62.316	–	–	–	–
Jaehnig et al.	2021	41.11	62.333	0.314	0.583	-0.224	–
Rain et al.	2021	41.106	62.327	0.293	0.585	-0.208	–
Dias et al.	2021	41.112	62.329	0.291	0.602	-0.203	–
Cantat-Gaudin et al.	2020	41.106	62.327	0.293	0.585	-0.208	–
Cantat-Gaudin & Anders	2020	41.106	62.327	0.293	0.585	-0.208	–
Bica et al.	2019	41.114	62.286	–	–	–	–
Cantat-Gaudin et al.	2018	41.106	62.327	0.293	0.585	-0.208	–
Loktin & Popova	2017	41.115	62.318	–	-0.083	-0.173	–
Kharchenko et al.	2016	41.102	62.316	–	–	–	–
Dias et al.	2014	41.175	62.35	–	-1.05	-2.21	–
Kharchenko et al.	2013	41.113	62.318	–	0.29	-0.32	–
Kharchenko et al.	2012	41.113	62.318	–	0.29	-0.32	–
van den Bergh	2006	41.175	62.35	–	–	–	–
Dias et al.	2002	41.175	62.35	–	-1.05	-2.21	–

💡 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	3.09	2.05	–	217	0.148	–	–	–
Almeida et al.	2025	2.75	2.19	–	86	–	720	–	–
Hunt & Reffert	2024	–	–	–	–	–	1382*	–	–
Cavallo et al.	2024	3.09	2.17	–	126	0.220	–	–	–
Hunt & Reffert	2023	3.05	1.87	1.05	117	–	–	–	–
Almeida et al.	2023	2.82	2.20	–	95	-0.163	850*	0.56	–
Just et al.	2023	–	–	–	7	–	376	–	–
Jaehnig et al.	2021	3.14*	–	–	–	–	–	–	–
Rain et al.	2021	3.10	2.33	–	7	–	–	–	0
Dias et al.	2021	2.75	2.19	–	86	-0.179	–	–	–
Cantat-Gaudin et al.	2020	3.50	1.83	–	240	–	–	–	–
Cantat-Gaudin & Anders	2020	3.10	–	–	–	–	–	–	–
Cantat-Gaudin et al.	2018	3.10	–	–	–	–	–	–	–
Loktin & Popova	2017	3.90	2.30	–	9	–	–	–	–
Kharchenko et al.	2016	4.10	2.94	–	7	–	–	–	–
Kharchenko et al.	2013	4.10	2.94	–	7	–	–	–	–
Kharchenko et al.	2012	4.10	2.94	–	7	–	–	–	–
van den Bergh	2006	3.96	2.36	–	7	–	–	–	–
Dias et al.	2002	3.96	2.34	–	7	–	–	–	–

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

Visualization

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