Collinder 183

(VDBH 28; NGC 2580; MWSC 1476; OCL 709; vdBergh-Hagen 28; ESO 431 06)

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0.90 UTI
0.75
CN
1.0
Cdens
1.0
CC3
0.87
Clit
1.0
Cdup
Stellar density (N50/rad) 5.2 [N/pc2]
  • CN 0.75 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.87 Well-studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Collinder 183 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is well-studied in the literature.

Almeida et al. (2025)
Mass determination: worst 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– 125.366 -30.307 0.214 -2.308 1.933 68.508
Li et al. 2025 125.371 -30.306 0.194 -2.307 1.91 –
Hu & Soubiran 2025 125.361 -30.312 – – – –
Almeida et al. 2025 125.367 -30.305 – – – –
Hunt & Reffert 2024 125.369 -30.305 0.222 -2.302 1.942 68.005
Cavallo et al. 2024 125.361 -30.312 0.224 – – –
Hunt & Reffert 2023 125.369 -30.305 0.222 -2.302 1.942 68.005
Just et al. 2023 125.372 -30.292 – – – –
Dias et al. 2021 125.367 -30.305 0.196 -2.293 1.898 66.704
Cantat-Gaudin et al. 2020 125.371 -30.306 0.194 -2.307 1.91 –
Cantat-Gaudin & Anders 2020 125.371 -30.306 0.194 -2.307 1.91 –
Soubiran et al. 2018 125.371 -30.306 – – – 67.39
Bica et al. 2019 125.371 -30.296 – – – –
Cantat-Gaudin et al. 2018 125.371 -30.306 0.194 -2.307 1.91 –
Kharchenko et al. 2016 125.372 -30.292 – – – –
Dias et al. 2014 125.367 -30.3 – -1.41 2.63 –
Kharchenko et al. 2013 125.377 -30.295 – -3.83 1.16 –
Dias et al. 2002 125.367 -30.3 – -1.41 2.63 –

💡 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– 4.295 0.58 1.17 522 -0.210 746 – –
Li et al. 2025 4.44 0.53 – 508 -0.060 – – –
Hu & Soubiran 2025 – – – – -0.290(5) – – –
Almeida et al. 2025 3.91 0.58 – 552 – 158 – –
Hunt & Reffert 2024 – – – – – 746(1) – –
Cavallo et al. 2024 2.74 0.95 – 741 -0.890 – – –
Hunt & Reffert 2023 4.12 0.23 1.17 904 – – – –
Just et al. 2023 – – – 251 – 1233 – –
Dias et al. 2021 3.91 0.58 – 552 -0.131 – – –
Cantat-Gaudin et al. 2020 4.15 0.32 – 537 – – – –
Cantat-Gaudin & Anders 2020 4.48 – – – – – – –
Soubiran et al. 2018 4.48 – – – – – – –
Cantat-Gaudin et al. 2018 4.48 – – – – – – –
Kharchenko et al. 2016 5.07 0.73 – 251 – – – –
Kharchenko et al. 2013 5.07 0.73 – 251 – – – –
Dias et al. 2002 4.00 0.87 – 158 – – – –

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

Visualization

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