Collinder 186
(VDBH 29; NGC 2588; MWSC 1480; OCL 715; vdBergh-Hagen 29; ESO 370 10)
0.90
UTI
0.75
CN
1.0
Cdens
1.0
CC3
0.87
Clit
1.0
Cdup
Stellar density (N50/rad)
16.2 [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 186 is a rich, very dense object of very high C3 quality. Its parallax locates it at a large 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 metallicity parameter (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 | 125.802 | -32.973 | 0.19 | -1.88 | 2.569 | 43.731 |
| Li et al. | 2025 | 125.797 | -32.972 | 0.199 | -1.884 | 2.521 | â |
| Hu & Soubiran | 2025 | 125.805 | -32.968 | â | â | â | â |
| Almeida et al. | 2025 | 125.799 | -32.968 | â | â | â | â |
| Hunt & Reffert | 2024 | 125.798 | -32.973 | 0.186 | -1.891 | 2.577 | 43.819 |
| Cavallo et al. | 2024 | 125.805 | -32.968 | 0.19 | â | â | â |
| Hunt & Reffert | 2023 | 125.798 | -32.973 | 0.186 | -1.891 | 2.577 | 43.819 |
| Just et al. | 2023 | 125.799 | -32.967 | â | â | â | â |
| Dias et al. | 2021 | 125.799 | -32.968 | 0.193 | -1.897 | 2.51 | â |
| Cantat-Gaudin et al. | 2020 | 125.797 | -32.972 | 0.199 | -1.884 | 2.521 | â |
| Cantat-Gaudin & Anders | 2020 | 125.797 | -32.972 | 0.199 | -1.884 | 2.521 | â |
| Bica et al. | 2019 | 125.793 | -32.975 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 125.797 | -32.972 | 0.199 | -1.884 | 2.521 | â |
| Kharchenko et al. | 2016 | 125.799 | -32.967 | â | â | â | â |
| Dias et al. | 2014 | 125.792 | -32.975 | â | -2.62 | 0.63 | â |
| Kharchenko et al. | 2013 | 125.805 | -32.97 | â | 0.04 | 3.17 | â |
| van den Bergh | 2006 | 125.8 | -32.983 | â | â | â | â |
| Dias et al. | 2002 | 125.792 | -32.975 | â | 0.04 | 3.17 | 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 | 4.39 | 0.93 | 0.78 | 517 | -0.191 | 310 | â | â |
| Li et al. | 2025 | 4.74 | 0.94 | â | 517 | 0.170 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.270(5) | â | â | â |
| Almeida et al. | 2025 | 4.30 | 1.24 | â | 398 | â | 310 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 759(1) | â | â |
| Cavallo et al. | 2024 | 3.58 | 1.29 | â | 562 | -0.240 | â | â | â |
| Hunt & Reffert | 2023 | 4.60 | 0.69 | 0.78 | 491 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 794 | â | 287 | â | â |
| Dias et al. | 2021 | 4.30 | 1.24 | â | 398 | -0.142 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 4.68 | 0.80 | â | 550 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.39 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.39 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 2.42 | 0.78 | â | 794 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.42 | 0.78 | â | 794 | â | â | â | â |
| van den Bergh | 2006 | 5.25 | 0.93 | â | 398 | â | â | â | â |
| Dias et al. | 2002 | 4.95 | 0.93 | â | 447 | 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: good fit. Isochrone match: intermediate fit. Silver sample.
Cavallo et al. (2024)
Gold sample.