Collinder 269
(MWSC 2113; OCL 897; ESO 096 10)
0.90
UTI
0.76
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
5.9 [arcmin]
- 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 269 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below 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 | 200.984 | -66.194 | 0.581 | -5.089 | -2.444 | -29.108 |
| Li et al. | 2025 | 200.992 | -66.204 | 0.568 | -5.058 | -2.492 | â |
| Hu & Soubiran | 2025 | 200.996 | -66.192 | â | â | â | â |
| Almeida et al. | 2025 | 201.022 | -66.212 | â | â | â | â |
| Hunt & Reffert | 2024 | 200.964 | -66.191 | 0.575 | -5.109 | -2.436 | -38.354 |
| Cavallo et al. | 2024 | 200.996 | -66.192 | 0.58 | â | â | â |
| Hunt & Reffert | 2023 | 200.964 | -66.191 | 0.575 | -5.109 | -2.436 | -38.354 |
| Almeida et al. | 2023 | 201.024 | -66.203 | â | â | â | â |
| Just et al. | 2023 | 200.952 | -66.157 | â | â | â | â |
| Dias et al. | 2021 | 201.022 | -66.212 | 0.572 | -5.059 | -2.478 | â |
| Cantat-Gaudin et al. | 2020 | 200.992 | -66.204 | 0.568 | -5.058 | -2.492 | â |
| Cantat-Gaudin & Anders | 2020 | 200.992 | -66.204 | 0.568 | -5.058 | -2.492 | â |
| Soubiran et al. | 2018 | 200.992 | -66.204 | â | â | â | -22.3 |
| Bica et al. | 2019 | 200.887 | -66.19 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 200.992 | -66.204 | 0.568 | -5.058 | -2.492 | â |
| Kharchenko et al. | 2016 | 200.952 | -66.157 | â | â | â | â |
| Dias et al. | 2014 | 200.879 | -66.183 | â | -3.45 | -3.87 | â |
| Kharchenko et al. | 2013 | 200.962 | -66.16 | â | -8.16 | -1.75 | â |
| Piskunov et al. | 2008 | 200.859 | -66.181 | â | â | â | â |
| Kharchenko et al. | 2005 | 200.88 | -66.18 | â | -7.95 | -3.93 | 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 | 1.35 | 0.62 | â | 918 | -0.242 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.280* | â | â | â |
| Almeida et al. | 2025 | 1.57 | 0.81 | â | 444 | â | 208 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 354* | â | â |
| Cavallo et al. | 2024 | 1.49 | 0.76 | â | 692 | -0.080 | â | â | â |
| Hunt & Reffert | 2023 | 1.62 | 0.61 | 0.28 | 409 | â | â | â | â |
| Almeida et al. | 2023 | 1.62 | 1.00 | â | 385 | 0.013 | 477* | 0.52 | â |
| Just et al. | 2023 | â | â | â | 355 | â | 676 | â | â |
| Dias et al. | 2021 | 1.57 | 0.81 | â | 444 | 0.205 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.71 | 0.78 | â | 417 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.68 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 1.68 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.68 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.87 | 1.35 | â | 355 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.87 | 1.35 | â | 355 | â | â | â | â |
| Piskunov et al. | 2008 | 1.30 | 0.84 | â | 331 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.30 | 0.84 | â | 331 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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