Czernik 1

(MWSC 17; OCL 283)

0.79 UTI

0.45

C_N

1.0

C_dens

0.5

C_C3

1.0

C_lit

1.0

C_dup

C3 classification BB

Number of members (P>50%) 45

Radius (P>50% members) 1.2 [arcmin]

C_N 0.45 Poorly populated
C_dens 1.0 Very dense
C_C3 0.5 Intermediate 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 1 is a poorly populated, very dense object of intermediate 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, but with a large variance across recent sources for the metallicity and mass parameters (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. Silver sample.

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for Czernik 1 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	–	1.904	61.483	0.313	-2.953	-1.449	–
Li et al.	2025	1.906	61.476	0.31	-2.964	-1.395	–
Almeida et al.	2025	1.907	61.477	–	–	–	–
Hunt & Reffert	2024	1.907	61.479	0.321	-2.949	-1.465	–
Cavallo et al.	2024	1.909	61.486	0.32	–	–	–
Hunt & Reffert	2023	1.907	61.479	0.321	-2.949	-1.465	–
Almeida et al.	2023	1.908	61.481	–	–	–	–
Just et al.	2023	1.893	61.486	–	–	–	–
Dias et al.	2021	1.907	61.477	0.308	-2.956	-1.379	–
Cantat-Gaudin et al.	2020	1.906	61.476	0.31	-2.964	-1.395	–
Cantat-Gaudin & Anders	2020	1.906	61.476	0.31	-2.964	-1.395	–
Bica et al.	2019	1.915	61.479	–	–	–	–
Cantat-Gaudin et al.	2018	1.906	61.476	0.31	-2.964	-1.395	–
Loktin & Popova	2017	1.905	61.475	–	-1.073	-0.342	–
Kharchenko et al.	2016	1.893	61.486	–	–	–	–
Kharchenko et al.	2013	1.902	61.49	–	-3.83	1.66	–
Kharchenko et al.	2012	1.902	61.49	–	-3.83	1.66	–
Dias et al.	2002	1.908	61.475	–	-3.83	1.66	–

💡 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	2.58	2.48	–	25	-0.065	–	–	–
Almeida et al.	2025	2.62	2.34	–	22	–	228	–	–
Hunt & Reffert	2024	–	–	–	–	–	510*	–	–
Cavallo et al.	2024	2.90	2.23	–	62	0.630	–	–	–
Hunt & Reffert	2023	2.88	2.35	0.80	68	–	–	–	–
Almeida et al.	2023	2.69	2.39	–	17	-0.079	201*	0.44	–
Just et al.	2023	–	–	–	58	–	22	–	–
Dias et al.	2021	2.62	2.34	–	22	-0.087	–	–	–
Cantat-Gaudin et al.	2020	3.12	2.17	–	37	–	–	–	–
Cantat-Gaudin & Anders	2020	2.95	–	–	–	–	–	–	–
Cantat-Gaudin et al.	2018	2.95	–	–	–	–	–	–	–
Loktin & Popova	2017	2.17	2.27	–	14	–	–	–	–
Kharchenko et al.	2016	2.61	2.58	–	58	–	–	–	–
Kharchenko et al.	2013	2.61	2.58	–	58	–	–	–	–
Kharchenko et al.	2012	2.61	2.58	–	58	–	–	–	–
Dias et al.	2002	2.53	3.81	–	5	–	–	–	–

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

Visualization

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