Czernik 14

(MWSC 267; OCL 376)

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0.85 UTI
0.77
CN
1.0
Cdens
0.75
CC3
0.86
Clit
1.0
Cdup
C3 classification AB
Number of members (P>50%) 143
Radius (P>50% members) 3.0 [arcmin]
  • CN 0.77 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.86 Well-studied
  • Cdup 1.0 Unique
đŸ“Ĩ Members 📊 Colab đŸ”Ŧ Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (Îą, δ) 🔍 Simbad (Îą, δ)

Overview
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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 well-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.

Data
🔍 Search references for Czernik 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 – 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 – – – –
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 –
Kharchenko et al. 2016 49.254 58.603 – – – –
Kharchenko et al. 2013 49.267 58.605 – 0.33 -2.46 –
Kharchenko et al. 2012 49.267 58.605 – 0.33 -2.46 –
Dias et al. 2002 49.225 58.6 – 0.33 -2.46 –

💡 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
Almeida et al. 2025 3.07 3.08 – 313 – 612 – –
Hunt & Reffert 2024 – – – – – 1799* – –
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 – –
Dias et al. 2021 3.07 3.08 – 313 0.000 – – –
Cantat-Gaudin et al. 2020 3.18 3.03 – 417 – – – –
Cantat-Gaudin & Anders 2020 3.18 – – – – – – –
Soubiran et al. 2018 3.18 – – – – – – –
Cantat-Gaudin et al. 2018 3.18 – – – – – – –
Loktin & Popova 2017 1.84 2.39 – 708 – – – –
Kharchenko et al. 2016 2.20 3.32 – 384 – – – –
Kharchenko et al. 2013 2.20 3.32 – 384 – – – –
Kharchenko et al. 2012 2.20 3.32 – 384 – – – –
Dias et al. 2002 2.17 5.30 – 251 – – – –

(*): Indicates that this parameter is assigned more than one value 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
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Czernik 14 UCC
Czernik 14 HUNT23
Czernik 14 CANTAT20
Galactocentric position diagram