Collinder 258
(Collinder 257; VDBH 133; vdB-Hagen 133; Harvard 5; Har5; OCL 880; vdBergh-Hagen 133; ESO 131 05; HD 108353; MWSC 2033; MWSC 2027; FoF 2240)
0.90
UTI
0.76
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
20.5 [N/pc2]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Collinder 258 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close 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 very 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 | 186.807 | -60.776 | 0.797 | -7.04 | -0.256 | -28.922 |
| Li et al. | 2025 | 186.798 | -60.767 | 0.764 | -7.051 | -0.288 | â |
| Almeida et al. | 2025 | 186.77 | -60.76 | â | â | â | â |
| Hunt & Reffert | 2024 | 186.789 | -60.769 | 0.795 | -7.02 | -0.249 | -30.848 |
| Cavallo et al. | 2024 | 186.786 | -60.771 | 0.8 | â | â | â |
| Hunt & Reffert | 2023 | 186.789 | -60.769 | 0.795 | -7.02 | -0.249 | -30.848 |
| Almeida et al. | 2023 | 186.735 | -60.761 | â | â | â | â |
| Cordoni et al. | 2023 | 186.77 | -60.76 | 0.765 | -7.065 | -0.263 | â |
| He et al. | 2022 | 186.766 | -60.769 | 0.801 | -7.026 | -0.254 | â |
| Tarricq et al. | 2022 | 186.82 | -60.767 | 0.797 | -7.031 | -0.263 | â |
| Jaehnig et al. | 2021 | 186.805 | -60.776 | 0.798 | -7.031 | -0.287 | â |
| Rain et al. | 2021 | 186.817 | -60.77 | 0.764 | -7.027 | -0.332 | â |
| Dias et al. | 2021 | 186.77 | -60.76 | 0.765 | -7.065 | -0.263 | â |
| Cantat-Gaudin et al. | 2020 | 186.798 | -60.767 | 0.764 | -7.051 | -0.288 | â |
| Cantat-Gaudin & Anders | 2020 | 186.798 | -60.767 | 0.764 | -7.051 | -0.288 | â |
| Liu & Pang | 2019 | 186.759 | -60.767 | 0.759 | -7.017 | -0.274 | â |
| Bossini et al. | 2019 | 186.808 | -60.769 | â | â | â | â |
| Soubiran et al. | 2018 | 186.798 | -60.767 | â | â | â | -28.0 |
| Bica et al. | 2019 | 186.809 | -60.773 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 186.798 | -60.767 | 0.764 | -7.051 | -0.288 | â |
| Loktin & Popova | 2017 | 186.81 | -60.779 | â | -13.683 | -7.13 | 14.9 |
| Dias et al. | 2014 | 186.192 | -60.887 | â | -4.35 | -1.17 | â |
| Gozha et al. | 2012 | 186.817 | -60.779 | â | â | â | â |
| Piskunov et al. | 2008 | 186.79 | -60.762 | â | â | â | â |
| van den Bergh | 2006 | 186.817 | -60.78 | â | â | â | â |
| Kharchenko et al. | 2005 | 186.79 | -60.77 | â | -7.81 | -0.73 | â |
| Kharchenko et al. | 2003 | 186.79 | -60.77 | â | -7.29 | -0.55 | â |
| Dias et al. | 2002 | 186.817 | -60.779 | â | -2.94 | -1.94 | 14.9 |
| Dambis | 1999 | 186.817 | -60.778 | â | â | â | 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 | 1.2 | 0.565 | 0.46 | 110 | 0.149 | 405 | 0.59 | 0.0 |
| Li et al. | 2025 | 1.19 | 0.60 | â | 192 | 0.149 | â | â | â |
| Almeida et al. | 2025 | 1.19 | 0.75 | â | 139 | â | 402 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 471(1) | â | â |
| Cavallo et al. | 2024 | 1.44 | 0.82 | â | 138 | 0.470 | â | â | â |
| Hunt & Reffert | 2023 | 1.18 | 0.62 | 0.46 | 160 | â | â | â | â |
| Almeida et al. | 2023 | 1.21 | 0.79 | â | 147 | -0.039 | 405(1) | 0.53 | â |
| Cordoni et al. | 2023 | 1.19 | 0.75 | â | 139 | 0.150 | 1032 | 0.65 | 0.00 |
| He et al. | 2022 | â | 0.85 | â | 112 | â | â | â | â |
| Tarricq et al. | 2022 | 1.23 | â | â | 81 | â | â | â | â |
| Jaehnig et al. | 2021 | 1.25(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 1.26 | 0.50 | â | 107 | â | â | â | 0 |
| Dias et al. | 2021 | 1.19 | 0.75 | â | 139 | 0.150 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.28 | 0.53 | â | 98 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.26 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 93 | 0.250 | â | â | â |
| Bossini et al. | 2019 | 1.25 | 0.67 | â | 67 | -0.045 | â | â | â |
| Soubiran et al. | 2018 | 1.26 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.26 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.22 | 0.50 | â | 108 | â | â | â | â |
| Gozha et al. | 2012 | 1.18 | â | â | 108 | -0.070 | 229 | â | â |
| Piskunov et al. | 2008 | 1.20 | 0.50 | â | 112 | â | â | â | â |
| van den Bergh | 2006 | 1.18 | 0.50 | â | 107 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.20 | 0.50 | â | 112 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.18 | 0.50 | â | â | â | â | â | â |
| Dias et al. | 2002 | 1.18 | 0.50 | â | 108 | 0.070 | â | â | â |
| Dambis | 1999 | 0.86 | 0.52 | â | 32 | 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: good fit. Gold sample.
Cavallo et al. (2024)
Gold sample.