Collinder 287
(VDBH 165; NGC 5749; MWSC 2256; OCL 930; vdBergh-Hagen 165; ESO 176 04; FoF 2346)
0.90
UTI
0.75
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
17.8 [N/pc2]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Collinder 287 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 moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age 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 | 222.191 | -54.501 | 0.892 | -2.758 | -3.054 | -23.592 |
| Li et al. | 2025 | 222.204 | -54.502 | 0.89 | -2.756 | -3.079 | â |
| Almeida et al. | 2025 | 222.173 | -54.512 | â | â | â | â |
| Hunt & Reffert | 2024 | 222.221 | -54.491 | 0.88 | -2.779 | -3.063 | -21.638 |
| Cavallo et al. | 2024 | 222.159 | -54.523 | 0.887 | â | â | â |
| Hunt & Reffert | 2023 | 222.221 | -54.491 | 0.88 | -2.779 | -3.063 | -21.638 |
| Almeida et al. | 2023 | 222.166 | -54.528 | â | â | â | â |
| Just et al. | 2023 | 222.183 | -54.483 | â | â | â | â |
| He et al. | 2022 | 222.224 | -54.502 | 0.9 | -2.758 | -3.045 | â |
| Tarricq et al. | 2022 | 222.314 | -54.488 | 0.899 | -2.764 | -3.057 | â |
| Jaehnig et al. | 2021 | 222.211 | -54.503 | 0.922 | -2.752 | -3.081 | â |
| Rain et al. | 2021 | 222.204 | -54.502 | 0.89 | -2.756 | -3.079 | â |
| Dias et al. | 2021 | 222.173 | -54.512 | 0.893 | -2.759 | -3.08 | â |
| Cantat-Gaudin et al. | 2020 | 222.204 | -54.502 | 0.89 | -2.756 | -3.079 | â |
| Cantat-Gaudin & Anders | 2020 | 222.204 | -54.502 | 0.89 | -2.756 | -3.079 | â |
| Liu & Pang | 2019 | 222.199 | -54.515 | 0.913 | -2.783 | -3.057 | â |
| Bossini et al. | 2019 | 222.204 | -54.502 | â | â | â | â |
| Soubiran et al. | 2018 | 222.204 | -54.502 | â | â | â | -18.04 |
| Bica et al. | 2019 | 222.226 | -54.502 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 222.204 | -54.502 | 0.89 | -2.756 | -3.079 | â |
| Loktin & Popova | 2017 | 222.225 | -54.499 | â | 1.328 | -5.371 | â |
| Kharchenko et al. | 2016 | 222.183 | -54.483 | â | â | â | â |
| Dias et al. | 2014 | 222.221 | -54.498 | â | -3.81 | -2.24 | â |
| Kharchenko et al. | 2013 | 222.195 | -54.485 | â | -1.05 | -3.44 | â |
| Piskunov et al. | 2008 | 222.218 | -54.493 | â | â | â | â |
| van den Bergh | 2006 | 222.225 | -54.5 | â | â | â | â |
| Kharchenko et al. | 2005 | 222.22 | -54.5 | â | 0.22 | -3.88 | â |
| Kharchenko et al. | 2003 | 222.22 | -54.5 | â | 0.52 | -3.91 | â |
| Dias et al. | 2002 | 222.221 | -54.498 | â | -1.75 | -3.36 | â |
| Dambis | 1999 | 222.225 | -54.5 | 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 | 1.06 | 1.16 | 0.67 | 71 | 0.058 | 266 | 0.55 | 0.0 |
| Li et al. | 2025 | 1.08 | 0.99 | â | 251 | 0.052 | â | â | â |
| Almeida et al. | 2025 | 1.06 | 1.18 | â | 103 | â | 256 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 338(1) | â | â |
| Cavallo et al. | 2024 | 1.11 | 1.11 | â | 200 | 0.260 | â | â | â |
| Hunt & Reffert | 2023 | 1.06 | 1.04 | 0.67 | 117 | â | â | â | â |
| Almeida et al. | 2023 | 1.07 | 1.18 | â | 132 | 0.027 | 276(1) | 0.55 | â |
| Just et al. | 2023 | â | â | â | 100 | â | 129 | â | â |
| He et al. | 2022 | â | 1.20 | â | 89 | â | â | â | â |
| Tarricq et al. | 2022 | 1.09 | â | â | 56 | â | â | â | â |
| Jaehnig et al. | 2021 | 1.09(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 1.09 | 1.02 | â | 65 | â | â | â | 0 |
| Dias et al. | 2021 | 1.06 | 1.18 | â | 103 | 0.063 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.12 | 0.90 | â | 52 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.09 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 63 | 0.500 | â | â | â |
| Bossini et al. | 2019 | 1.18 | 1.02 | â | 65 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 1.09 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.09 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.03 | 1.16 | â | 54 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.01 | 1.48 | â | 100 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.01 | 1.48 | â | 100 | â | â | â | â |
| Piskunov et al. | 2008 | 1.03 | 1.15 | â | 26 | â | â | â | â |
| van den Bergh | 2006 | 1.03 | 1.18 | â | 54 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.03 | 1.15 | â | 26 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.03 | 1.12 | â | â | â | â | â | â |
| Dias et al. | 2002 | 1.03 | 1.17 | â | 53 | â | â | â | â |
| Dambis | 1999 | 0.91 | 1.25 | â | 71 | 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.
Cavallo et al. (2024)
Gold sample.