Czernik 24

(FSR 0881; MWSC 695; OCL 472)

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0.91 UTI
0.79
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
C3 classification AB
Number of members (P>50%) 197
Radius (P>50% members) 2.6 [arcmin]
  • CN 0.79 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 1.0 Very well-studied
  • Cdup 1.0 Unique
πŸ“₯ Members πŸ“Š Colab πŸ”¬ Bayestar19 πŸ” CDS πŸ” Simbad πŸ” CDS (Ξ±, Ξ΄) πŸ” Simbad (Ξ±, Ξ΄)

Overview
ℹ️
Czernik 24 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, old cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is very well-studied in the literature.
Distant Moderate extinction Massive Near-solar metallicity Old

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

Cavallo et al. (2024)
Gold sample.

Data
πŸ” Search references for Czernik 24 in: SciX Simbad
ℹ️
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 88.848 20.877 0.236 0.256 -2.704 20.991
Hu & Soubiran 2025 88.847 20.875 – – – –
Almeida et al. 2025 88.832 20.873 – – – –
Hunt & Reffert 2024 88.852 20.877 0.228 0.26 -2.721 16.008
Cavallo et al. 2024 88.847 20.875 0.225 – – –
Hunt & Reffert 2023 88.852 20.877 0.228 0.26 -2.721 16.008
Just et al. 2023 88.852 20.886 – – – –
Dias et al. 2021 88.832 20.873 0.201 0.253 -2.668 –
Cantat-Gaudin et al. 2020 88.848 20.876 0.261 0.222 -2.629 –
SΓ‘nchez et al. 2020 88.854 20.886 – 0.353 -2.589 –
Cantat-Gaudin & Anders 2020 88.848 20.876 0.261 0.222 -2.629 –
Soubiran et al. 2018 88.848 20.876 – – – 30.1
Bica et al. 2019 88.855 20.878 – – – –
Cantat-Gaudin et al. 2018 88.848 20.876 0.261 0.222 -2.629 –
Loktin & Popova 2017 88.86 20.887 – 0.9 -2.194 –
Kharchenko et al. 2016 88.852 20.886 – – – –
Dias et al. 2014 88.854 20.886 – 1.79 -4.31 –
Kharchenko et al. 2013 88.86 20.885 – 2.81 -6.33 –
Glushkova et al. 2010 88.853 20.886 – – – –
Froebrich et al. 2007 88.854 20.883 – – – –
Dias et al. 2002 88.854 20.886 – 1.79 -4.31 –

πŸ’‘ 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
Hu & Soubiran 2025 – – – – -0.210* – – –
Almeida et al. 2025 3.62 2.31 – 1343 – 474 – –
Hunt & Reffert 2024 – – – – – 1071* – –
Cavallo et al. 2024 3.37 1.72 – 2455 0.250 – – –
Hunt & Reffert 2023 3.82 1.97 0.93 1202 – – – –
Just et al. 2023 – – – 1259 – 1042 – –
Dias et al. 2021 3.62 2.31 – 1343 -0.297 – – –
Cantat-Gaudin et al. 2020 3.98 1.63 – 2692 – – – –
Cantat-Gaudin & Anders 2020 3.45 – – – – – – –
Soubiran et al. 2018 3.45 – – – – – – –
Cantat-Gaudin et al. 2018 3.45 – – – – – – –
Loktin & Popova 2017 3.67 2.06 – 158 – – – –
Kharchenko et al. 2016 5.04 1.81 – 1259 – – – –
Kharchenko et al. 2013 5.04 1.81 – 1259 – – – –
Glushkova et al. 2010 4.60 0.81 – 2512 – – – –
Dias et al. 2002 4.60 0.81 – 2512 – – – –

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

Visualization
ℹ️
Czernik 24 UCC
Czernik 24 HUNT23
Czernik 24 CANTAT20
Galactocentric position diagram