Czernik 4

(MWSC 126)

0.25 UTI

0.25

C_N

0.12

C_dens

0.12

C_C3

0.38

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 25

Radius (P>50% members) 6.9 [arcmin]

C_N 0.25 Poorly populated
C_dens 0.12 Very loose
C_C3 0.12 Very low quality
C_lit 0.38 Poorly studied
C_dup 1.0 Unique

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

Overview

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Czernik 4 is a poorly populated, very loose object of very low C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane, affected by high extinction. It is catalogued as a low-mass, young cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~3.16 kpc) differs significantly from the median photometric distance (~1.63 kpc).

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close High extinction Low mass Young

Data

🔍 Search references for Czernik 4 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	–	23.886	61.493	0.316	-2.289	-0.352	-49.201
Just et al.	2023	23.891	61.461	–	–	–	–
Loktin & Popova	2017	23.895	61.476	–	1.987	-2.909	-11.4
Kharchenko et al.	2016	23.891	61.461	–	–	–	–
Kharchenko et al.	2013	23.902	61.463	–	1.84	-1.84	-11.4
Kharchenko et al.	2012	23.902	61.463	–	0.13	-3.9	–
Dias et al.	2002	23.9	61.476	–	0.13	-3.9	-11.4

💡 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
Just et al.	2023	–	–	–	52	–	16	–	–
Loktin & Popova	2017	2.18	1.22	–	100	–	–	–	–
Kharchenko et al.	2016	1.63	3.10	–	52	–	–	–	–
Kharchenko et al.	2013	1.63	3.10	–	52	–	–	–	–
Kharchenko et al.	2012	1.70	3.10	–	132	–	–	–	–
Dias et al.	2002	1.63	3.29	–	100	–	–	–	–

Visualization

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