Collinder 237
(VDBH 108; NGC 3496; MWSC 1878; OCL 836; vdBergh-Hagen 108; ESO 128 26; FSR 1562; FoF 236)
1.0
UTI
1.0
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
57.3 [N/pc2]
- CN 1.0 Very rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Collinder 237 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is very well-studied in the literature.
Note: This object contains blue stragglers according to at least one source.
Note: This object shares a very small percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 164.871 | -60.335 | 0.403 | -7.411 | 2.716 | 8.816 |
| Li et al. | 2025 | 164.877 | -60.335 | 0.391 | -7.408 | 2.668 | β |
| Carrasco-Varela et al. | 2025 | 165.012 | -60.451 | β | β | β | β |
| Almeida et al. | 2025 | 164.881 | -60.336 | β | β | β | β |
| Hunt & Reffert | 2024 | 164.877 | -60.332 | 0.406 | -7.414 | 2.722 | 8.026 |
| Cavallo et al. | 2024 | 164.876 | -60.339 | 0.405 | β | β | β |
| Hunt & Reffert | 2023 | 164.877 | -60.332 | 0.406 | -7.414 | 2.722 | 8.026 |
| Almeida et al. | 2023 | 164.873 | -60.336 | β | β | β | β |
| Just et al. | 2023 | 164.896 | -60.337 | β | β | β | β |
| Jaehnig et al. | 2021 | 164.878 | -60.334 | 0.423 | -7.406 | 2.688 | β |
| Rain et al. | 2021 | 164.877 | -60.335 | 0.391 | -7.408 | 2.668 | β |
| Dias et al. | 2021 | 164.881 | -60.336 | 0.392 | -7.402 | 2.671 | 9.611 |
| Cantat-Gaudin et al. | 2020 | 164.877 | -60.335 | 0.391 | -7.408 | 2.668 | β |
| SΓ‘nchez et al. | 2020 | 164.9 | -60.337 | β | -7.391 | 2.72 | β |
| Cantat-Gaudin & Anders | 2020 | 164.877 | -60.335 | 0.391 | -7.408 | 2.668 | β |
| Liu & Pang | 2019 | 164.869 | -60.325 | 0.389 | -7.305 | 2.644 | β |
| Bossini et al. | 2019 | 164.877 | -60.335 | β | β | β | β |
| Soubiran et al. | 2018 | 164.877 | -60.335 | β | β | β | 9.62 |
| Bica et al. | 2019 | 164.911 | -60.338 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 164.877 | -60.335 | 0.391 | -7.408 | 2.668 | β |
| Loktin & Popova | 2017 | 164.895 | -60.336 | β | -3.61 | -1.14 | -6.3 |
| Kharchenko et al. | 2016 | 164.896 | -60.337 | β | β | β | β |
| Dias et al. | 2014 | 164.9 | -60.337 | β | -3.61 | -1.14 | β |
| Kharchenko et al. | 2013 | 164.902 | -60.34 | β | -7.62 | 4.17 | -6.3 |
| Gozha et al. | 2012 | 164.9 | -60.337 | β | β | β | β |
| Piskunov et al. | 2008 | 164.887 | -60.387 | β | β | β | β |
| Kharchenko et al. | 2007 | 164.89 | -60.34 | β | 0.15 | β | -51.4 |
| van den Bergh | 2006 | 164.9 | -60.383 | β | β | β | β |
| Kharchenko et al. | 2005 | 164.89 | -60.39 | β | -7.3 | 2.08 | -51.4 |
| Kharchenko et al. | 2003 | 165.12 | -60.32 | β | -8.35 | 1.95 | β |
| Dias et al. | 2002 | 164.9 | -60.337 | β | -3.61 | -1.14 | -51.4 |
π‘ 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 | 99999β | 2.05 | 1.455 | 1.46 | 472 | 0.130 | 1785 | 0.63 | 0.02 |
| Li et al. | 2025 | 2.23 | 1.34 | β | 653 | 0.259 | β | β | β |
| Carrasco-Varela et al. | 2025 | 2.05 | 1.62 | β | 564 | 0.050 | β | β | 0.02(1) |
| Almeida et al. | 2025 | 2.05 | 1.62 | β | 564 | β | 1785 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 4506(1) | β | β |
| Cavallo et al. | 2024 | 2.23 | 1.75 | β | 417 | 0.280 | β | β | β |
| Hunt & Reffert | 2023 | 2.26 | 1.45 | 1.46 | 352 | β | β | β | β |
| Almeida et al. | 2023 | 2.16 | 1.55 | β | 542 | 0.153 | 2044(1) | 0.63 | β |
| Just et al. | 2023 | β | β | β | 785 | β | 143 | β | β |
| Jaehnig et al. | 2021 | 2.34(1) | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 2.38 | 1.43 | β | 295 | β | β | β | 0 |
| Dias et al. | 2021 | 2.05 | 1.62 | β | 564 | 0.130 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 2.31 | 1.27 | β | 501 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 2.38 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 1410 | -0.500 | β | β | β |
| Bossini et al. | 2019 | 2.48 | 1.45 | β | 443 | 0.000 | β | β | β |
| Soubiran et al. | 2018 | 2.38 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 2.38 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 0.99 | 1.45 | β | 296 | β | β | β | β |
| Kharchenko et al. | 2016 | 1.36 | 1.29 | β | 785 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.36 | 1.29 | β | 785 | β | β | β | β |
| Gozha et al. | 2012 | 0.99 | β | β | 296 | β | 200 | β | β |
| Piskunov et al. | 2008 | 0.99 | 1.46 | β | 417 | β | β | β | β |
| van den Bergh | 2006 | 0.99 | 1.46 | β | 295 | β | β | β | β |
| Kharchenko et al. | 2005 | 0.99 | 1.46 | β | 417 | β | β | β | β |
| Kharchenko et al. | 2003 | 0.99 | 1.46 | β | β | β | β | β | β |
| Dias et al. | 2002 | 0.99 | 1.45 | β | 296 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


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