Collinder 183
(VDBH 28; NGC 2580; MWSC 1476; OCL 709; vdBergh-Hagen 28; ESO 431 06)
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
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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 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 | â |
| Hu & Soubiran | 2025 | 125.361 | -30.312 | â | â | â | â |
| Almeida et al. | 2025 | 125.367 | -30.305 | â | â | â | â |
| 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 | â | â | â |
| Hunt & Reffert | 2023 | 125.369 | -30.305 | 0.222 | -2.302 | 1.942 | 68.005 |
| Just et al. | 2023 | 125.372 | -30.292 | â | â | â | â |
| 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 | â |
| Cantat-Gaudin & Anders | 2020 | 125.371 | -30.306 | 0.194 | -2.307 | 1.91 | â |
| Soubiran et al. | 2018 | 125.371 | -30.306 | â | â | â | 67.39 |
| Bica et al. | 2019 | 125.371 | -30.296 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 125.371 | -30.306 | 0.194 | -2.307 | 1.91 | â |
| Kharchenko et al. | 2016 | 125.372 | -30.292 | â | â | â | â |
| Dias et al. | 2014 | 125.367 | -30.3 | â | -1.41 | 2.63 | â |
| Kharchenko et al. | 2013 | 125.377 | -30.295 | â | -3.83 | 1.16 | â |
| Dias et al. | 2002 | 125.367 | -30.3 | â | -1.41 | 2.63 | â |
đĄ 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 | 99999â | 4.295 | 0.58 | 1.17 | 522 | -0.210 | 746 | â | â |
| Li et al. | 2025 | 4.44 | 0.53 | â | 508 | -0.060 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.290(5) | â | â | â |
| Almeida et al. | 2025 | 3.91 | 0.58 | â | 552 | â | 158 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 746(1) | â | â |
| Cavallo et al. | 2024 | 2.74 | 0.95 | â | 741 | -0.890 | â | â | â |
| Hunt & Reffert | 2023 | 4.12 | 0.23 | 1.17 | 904 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 251 | â | 1233 | â | â |
| Dias et al. | 2021 | 3.91 | 0.58 | â | 552 | -0.131 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 4.15 | 0.32 | â | 537 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.48 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 4.48 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.48 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 5.07 | 0.73 | â | 251 | â | â | â | â |
| Kharchenko et al. | 2013 | 5.07 | 0.73 | â | 251 | â | â | â | â |
| Dias et al. | 2002 | 4.00 | 0.87 | â | 158 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: worst fit. Isochrone match: intermediate fit.
Cavallo et al. (2024)
Gold sample.