Collinder 185
(MWSC 1481)
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
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
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 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 | â |
| Almeida et al. | 2025 | 125.818 | -36.346 | â | â | â | â |
| 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 | â | â | â |
| Hunt & Reffert | 2023 | 125.827 | -36.357 | 0.643 | -4.939 | 3.873 | 28.179 |
| Almeida et al. | 2023 | 125.828 | -36.368 | â | â | â | â |
| Just et al. | 2023 | 125.83 | -36.327 | â | â | â | â |
| Jaehnig et al. | 2021 | 125.831 | -36.349 | 0.65 | -5.005 | 3.855 | â |
| Rain et al. | 2021 | 125.833 | -36.349 | 0.626 | -4.924 | 3.879 | â |
| Dias et al. | 2021 | 125.818 | -36.346 | 0.63 | -4.913 | 3.888 | â |
| Cantat-Gaudin et al. | 2020 | 125.833 | -36.349 | 0.626 | -4.924 | 3.879 | â |
| Cantat-Gaudin & Anders | 2020 | 125.833 | -36.349 | 0.626 | -4.924 | 3.879 | â |
| Bossini et al. | 2019 | 125.833 | -36.349 | â | â | â | â |
| Soubiran et al. | 2018 | 125.833 | -36.349 | â | â | â | 75.78 |
| Cantat-Gaudin et al. | 2018 | 125.833 | -36.349 | 0.626 | -4.924 | 3.879 | â |
| Kharchenko et al. | 2016 | 125.83 | -36.327 | â | â | â | â |
| Dias et al. | 2014 | 125.838 | -36.333 | â | -3.48 | 1.39 | â |
| Kharchenko et al. | 2013 | 125.835 | -36.33 | â | -5.61 | 4.01 | â |
| Piskunov et al. | 2008 | 125.837 | -36.327 | â | â | â | â |
| van den Bergh | 2006 | 125.825 | -36.333 | â | â | â | â |
| Kharchenko et al. | 2005 | 125.83 | -36.33 | â | -6.53 | 2.83 | â |
| Kharchenko et al. | 2003 | 125.83 | -36.37 | â | -6.84 | 2.91 | â |
| Dias et al. | 2002 | 125.838 | -36.333 | â | -2.81 | 3.72 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 1.33 | 0.51 | â | 250 | -0.060 | â | â | â |
| Almeida et al. | 2025 | 1.42 | 0.65 | â | 104 | â | 170 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 372* | â | â |
| Cavallo et al. | 2024 | 1.43 | 0.67 | â | 110 | 0.180 | â | â | â |
| Hunt & Reffert | 2023 | 1.46 | 0.53 | 0.67 | 106 | â | â | â | â |
| Almeida et al. | 2023 | 1.44 | 0.76 | â | 109 | -0.031 | 245* | 0.52 | â |
| Just et al. | 2023 | â | â | â | 151 | â | 42 | â | â |
| Jaehnig et al. | 2021 | 1.52* | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 1.53 | 0.65 | â | 129 | â | â | â | 0 |
| Dias et al. | 2021 | 1.42 | 0.65 | â | 104 | 0.103 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.56 | 0.61 | â | 62 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.53 | â | â | â | â | â | â | â |
| Bossini et al. | 2019 | 1.57 | 0.69 | â | 50 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 1.53 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.53 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.48 | 0.78 | â | 151 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.48 | 0.78 | â | 151 | â | â | â | â |
| Piskunov et al. | 2008 | 1.49 | 0.65 | â | 151 | â | â | â | â |
| van den Bergh | 2006 | 1.49 | 0.65 | â | 129 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.49 | 0.65 | â | 151 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.49 | 0.65 | â | â | â | â | â | â |
| Dias et al. | 2002 | 1.49 | 0.65 | â | 129 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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