Czernik 14

(MWSC 267; OCL 376)

0.77 UTI

0.77

C_N

1.0

C_dens

0.75

C_C3

0.68

C_lit

1.0

C_dup

N_m (P>50%) 143

Core radius and density 1.1 [pc], 7.7 [pc^-2]

C3 classification AB

C_N 0.77 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.68 Moderately studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

ℹ️

Czernik 14 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is moderately studied in the literature.

Note: This object shares a small percentage of members with a later reported entry. See table with shared members information.

Distant High extinction Near-solar metallicity Intermediate age

Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.86 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.86 (50th percentile).

Hu et al. (2021)
Ellipticities (core, all): e_core=0.2216, e_all=0.0661.

Data

🔍 Search references for Czernik 14 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	49.272	58.611	0.299	-0.507	-0.453	-55.135
Almeida et al.	2025	49.258	58.613	–	–	–	–
Hunt & Reffert	2024	49.268	58.613	0.313	-0.455	-0.458	-38.819
Cavallo et al.	2024	49.286	58.59	0.304	–	–	–
Hunt & Reffert	2023	49.268	58.613	0.313	-0.455	-0.458	-38.819
Just et al.	2023	49.254	58.603	–	–	–	–
Jadhav & Subramaniam	2021	49.262	58.612	–	–	–	–
Dias et al.	2021	49.258	58.613	0.285	-0.463	-0.392	-55.53
Cantat-Gaudin et al.	2020	49.262	58.612	0.285	-0.49	-0.395	–
Cantat-Gaudin & Anders	2020	49.262	58.612	0.285	-0.49	-0.395	–
Soubiran et al.	2018	49.262	58.612	–	–	–	-55.7
Bica et al.	2019	49.231	58.602	–	–	–	–
Cantat-Gaudin et al.	2018	49.262	58.612	0.285	-0.49	-0.395	–
Loktin & Popova	2017	49.23	58.6	–	-0.284	-2.041	–
Sampedro et al.	2017	49.225	58.6	–	-0.88	-3.23	–
Kharchenko et al.	2016	49.254	58.603	–	–	–	–
Tadross	2014	49.225	58.6	–	–	–	–
Kharchenko et al.	2013	49.267	58.605	–	0.33	-2.46	–
Kharchenko et al.	2012	49.267	58.605	–	0.33	-2.46	–
Bukowiecki et al.	2011	49.263	58.611	–	–	–	–
Dias et al.	2002	49.225	58.6	–	0.33	-2.46	–
Lynga	1987	49.231	58.602	–	–	–	–

💡 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]	B_frac	BSS
UCC	99999–	3.015	3.38	2.09	384	0.105	837	–	0
Almeida et al.	2025	3.07	3.08	–	313	–	612	–	–
Hunt & Reffert	2024	2.96	3.55	2.09	243	–	1799⁽¹⁾	–	–
Cavallo et al.	2024	3.16	3.51	–	389	0.210	–	–	–
Hunt & Reffert	2023	2.96	3.55	2.09	243	–	–	–	–
Just et al.	2023	–	–	–	384	–	36	–	–
Jadhav & Subramaniam	2021	3.18	3.03	–	417	–	837	–	0⁽¹⁾
Dias et al.	2021	3.07	3.08	–	313	0.000	–	–	–
Cantat-Gaudin et al.	2020	3.18	3.03	–	417	–	–	–	–
Kounkel et al.	2020	3.25	3.13	–	398	–	–	–	–
Cantat-Gaudin & Anders	2020	3.18	–	–	–	–	–	–	–
Soubiran et al.	2018	3.18	–	–	–	–	–	–	–
Cantat-Gaudin et al.	2018	3.18	–	–	–	–	–	–	–
Loktin & Popova	2017	1.84	2.43	–	708	–	–	–	–
Kharchenko et al.	2016	2.20	3.38	–	384	–	–	–	–
Tadross	2014	2.17	5.39	–	250	–	–	–	–
Kharchenko et al.	2013	2.20	3.38	–	384	–	–	–	–
Bukowiecki et al.	2012	–	–	–	–	–	845	–	–
Kharchenko et al.	2012	2.20	3.38	–	384	–	–	–	–
Bukowiecki et al.	2011	2.92⁽¹⁾	3.31	–	8	–	–	–	–
Dias et al.	2002	2.17	5.39	–	251	–	–	–	–

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0261	18.9	49.26	58.61	0.29	-0.54	-0.45	9.35	0.0

💡 Note: The % column shows the percentage of members that Czernik 14 shares with each listed object.

Visualization

ℹ️

1 2 3