Collinder 94

(NGC 2236; MWSC 881; OCL 501; FSR 1002; FoF 80)

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0.95 UTI
1.0
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad) 38.7 [N/pc2]
  • CN 1.0 Very rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 1.0 Very well-studied
  • Cdup 1.0 Unique

Overview

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Collinder 94 is a very 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, intermediate-age cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is very well-studied in the literature.

Note: This object contains blue stragglers according to at least one source.

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

Almeida et al. (2025)
Mass determination: good fit. Isochrone match: intermediate fit.

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 97.415 6.834 0.342 -0.78 0.025 59.679
Li et al. 2025 97.416 6.834 0.35 -0.752 0.01 –
Hu & Soubiran 2025 97.417 6.834 – – – –
Carrasco-Varela et al. 2025 97.641 6.791 – – – –
Almeida et al. 2025 97.421 6.838 – – – –
Hunt & Reffert 2024 97.411 6.831 0.348 -0.782 0.016 59.296
Cavallo et al. 2024 97.417 6.834 0.347 – – –
Hunt & Reffert 2023 97.411 6.831 0.348 -0.782 0.016 59.296
Almeida et al. 2023 97.423 6.843 – – – –
Just et al. 2023 97.41 6.818 – – – –
Jaehnig et al. 2021 97.409 6.839 0.384 -0.765 0.041 –
Rain et al. 2021 97.416 6.834 0.35 -0.752 0.01 –
Dias et al. 2021 97.421 6.838 0.36 -0.754 -0.003 59.362
Cantat-Gaudin et al. 2020 97.416 6.834 0.35 -0.752 0.01 –
SΓ‘nchez et al. 2020 97.412 6.83 – -0.654 -0.048 –
Cantat-Gaudin & Anders 2020 97.416 6.834 0.35 -0.752 0.01 –
Liu & Pang 2019 97.422 6.83 0.36 -0.685 0.028 –
Soubiran et al. 2018 97.416 6.834 – – – 59.91
Bica et al. 2019 97.43 6.839 – – – –
Cantat-Gaudin et al. 2018 97.416 6.834 0.35 -0.752 0.01 –
Loktin & Popova 2017 97.41 6.831 – -2.37 -0.31 –
Kharchenko et al. 2016 97.41 6.818 – – – –
Dias et al. 2014 97.412 6.83 – -2.37 -0.31 –
Kharchenko et al. 2013 97.417 6.817 – -1.95 -1.41 –
Gozha et al. 2012 97.412 6.83 – – – –
van den Bergh 2006 97.425 6.833 – – – –
Dias et al. 2002 97.412 6.83 – -2.37 -0.31 –

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] Bfrac BSS
UCC 99999– 2.64 1.515 1.12 845 -0.150 1897 0.59 0.05
Li et al. 2025 2.77 1.54 – 845 -0.055 – – –
Hu & Soubiran 2025 – – – – -0.150(5) – – –
Carrasco-Varela et al. 2025 2.42 1.65 – 893 -0.150 – – 0.05(1)
Almeida et al. 2025 2.42 1.65 – 893 – 2463 – –
Hunt & Reffert 2024 – – – – – 3492(1) – –
Cavallo et al. 2024 2.37 1.49 – 1072 -0.070 – – –
Hunt & Reffert 2023 2.56 1.38 1.12 853 – – – –
Almeida et al. 2023 2.42 1.67 – 899 -0.153 1331(1) 0.59 –
Just et al. 2023 – – – 562 – 213 – –
Jaehnig et al. 2021 2.61(1) – – – – – – –
Rain et al. 2021 2.64 1.46 – 339 – – – 0
Dias et al. 2021 2.42 1.65 – 893 -0.100 – – –
Cantat-Gaudin et al. 2020 2.43 1.05 – 1148 – – – –
Cantat-Gaudin & Anders 2020 2.64 – – – – – – –
Liu & Pang 2019 – – – 1180 -0.250 – – –
Soubiran et al. 2018 2.64 – – – – – – –
Cantat-Gaudin et al. 2018 2.64 – – – – – – –
Loktin & Popova 2017 2.97 1.46 – 365 – – – –
Kharchenko et al. 2016 2.65 1.74 – 562 – – – –
Kharchenko et al. 2013 2.65 1.74 – 562 – – – –
Gozha et al. 2012 2.93 – – 345 -0.300 – – –
van den Bergh 2006 2.93 1.49 – 347 – – – –
Dias et al. 2002 2.93 1.48 – 345 -0.300 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Teutsch J0628.8+0708 0.1 97.25 7.15 0.26 -0.3 -0.2 – 0.05

πŸ’‘ Note: The % column shows the percentage of members that Collinder 94 shares with each listed object.

Visualization

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