Collinder 185

(MWSC 1481)

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0.90 UTI
0.74
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members) 6.9 [arcmin]
  • CN 0.74 Moderately populated
  • 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 185 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is very well-studied in the literature.
Relatively close Low extinction Near-solar metallicity Intermediate age

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

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 – 125.831 -36.365 0.644 -4.948 3.88 32.28
Li et al. 2025 125.833 -36.349 0.626 -4.924 3.879 –
Almeida et al. 2025 125.818 -36.346 – – – –
Hunt & Reffert 2024 125.827 -36.357 0.643 -4.939 3.873 28.179
Cavallo et al. 2024 125.911 -36.421 0.643 – – –
Hunt & Reffert 2023 125.827 -36.357 0.643 -4.939 3.873 28.179
Almeida et al. 2023 125.828 -36.368 – – – –
Just et al. 2023 125.83 -36.327 – – – –
Jaehnig et al. 2021 125.831 -36.349 0.65 -5.005 3.855 –
Rain et al. 2021 125.833 -36.349 0.626 -4.924 3.879 –
Dias et al. 2021 125.818 -36.346 0.63 -4.913 3.888 –
Cantat-Gaudin et al. 2020 125.833 -36.349 0.626 -4.924 3.879 –
Cantat-Gaudin & Anders 2020 125.833 -36.349 0.626 -4.924 3.879 –
Bossini et al. 2019 125.833 -36.349 – – – –
Soubiran et al. 2018 125.833 -36.349 – – – 75.78
Cantat-Gaudin et al. 2018 125.833 -36.349 0.626 -4.924 3.879 –
Kharchenko et al. 2016 125.83 -36.327 – – – –
Dias et al. 2014 125.838 -36.333 – -3.48 1.39 –
Kharchenko et al. 2013 125.835 -36.33 – -5.61 4.01 –
Piskunov et al. 2008 125.837 -36.327 – – – –
van den Bergh 2006 125.825 -36.333 – – – –
Kharchenko et al. 2005 125.83 -36.33 – -6.53 2.83 –
Kharchenko et al. 2003 125.83 -36.37 – -6.84 2.91 –
Dias et al. 2002 125.838 -36.333 – -2.81 3.72 –

💡 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
Li et al. 2025 1.33 0.51 – 250 -0.060 – – –
Almeida et al. 2025 1.42 0.65 – 104 – 170 – –
Hunt & Reffert 2024 – – – – – 372* – –
Cavallo et al. 2024 1.43 0.67 – 110 0.180 – – –
Hunt & Reffert 2023 1.46 0.53 0.67 106 – – – –
Almeida et al. 2023 1.44 0.76 – 109 -0.031 245* 0.52 –
Just et al. 2023 – – – 151 – 42 – –
Jaehnig et al. 2021 1.52* – – – – – – –
Rain et al. 2021 1.53 0.65 – 129 – – – 0
Dias et al. 2021 1.42 0.65 – 104 0.103 – – –
Cantat-Gaudin et al. 2020 1.56 0.61 – 62 – – – –
Cantat-Gaudin & Anders 2020 1.53 – – – – – – –
Bossini et al. 2019 1.57 0.69 – 50 0.000 – – –
Soubiran et al. 2018 1.53 – – – – – – –
Cantat-Gaudin et al. 2018 1.53 – – – – – – –
Kharchenko et al. 2016 1.48 0.78 – 151 – – – –
Kharchenko et al. 2013 1.48 0.78 – 151 – – – –
Piskunov et al. 2008 1.49 0.65 – 151 – – – –
van den Bergh 2006 1.49 0.65 – 129 – – – –
Kharchenko et al. 2005 1.49 0.65 – 151 – – – –
Kharchenko et al. 2003 1.49 0.65 – – – – – –
Dias et al. 2002 1.49 0.65 – 129 – – – –

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

Visualization

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