Collinder 437
(NGC 7086; MWSC 3520; OCL 214; FSR 0309; FoF 343)
1.0
UTI
1.0
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
94.9 [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 437 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close 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 metallicity and mass parameters (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 | 99999β | 322.623 | 51.593 | 0.598 | -1.654 | -1.659 | -19.182 |
| Wei et al. | 2025 | 322.622 | 51.593 | 0.599 | -1.652 | -1.671 | β |
| Almeida et al. | 2025 | 322.624 | 51.589 | β | β | β | β |
| Zhang et al. | 2024 | 322.628 | 51.595 | β | β | β | β |
| Hunt & Reffert | 2024 | 322.628 | 51.595 | 0.6 | -1.652 | -1.664 | -16.098 |
| Cavallo et al. | 2024 | 322.629 | 51.586 | 0.6 | β | β | β |
| Hunt & Reffert | 2023 | 322.628 | 51.595 | 0.6 | -1.652 | -1.664 | -16.098 |
| Almeida et al. | 2023 | 322.606 | 51.592 | β | β | β | β |
| Just et al. | 2023 | 322.607 | 51.604 | β | β | β | β |
| Jaehnig et al. | 2021 | 322.626 | 51.599 | 0.621 | -1.655 | -1.623 | β |
| Rain et al. | 2021 | 322.624 | 51.593 | 0.59 | -1.656 | -1.629 | β |
| Dias et al. | 2021 | 322.624 | 51.589 | 0.586 | -1.644 | -1.626 | -17.964 |
| Cantat-Gaudin et al. | 2020 | 322.624 | 51.593 | 0.59 | -1.656 | -1.629 | β |
| SΓ‘nchez et al. | 2020 | 322.613 | 51.6 | β | -1.539 | -1.74 | β |
| Cantat-Gaudin & Anders | 2020 | 322.624 | 51.593 | 0.59 | -1.656 | -1.629 | β |
| Liu & Pang | 2019 | 322.623 | 51.588 | 0.587 | -1.649 | -1.642 | β |
| Soubiran et al. | 2018 | 322.624 | 51.593 | β | β | β | -22.34 |
| Bica et al. | 2019 | 322.627 | 51.581 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 322.624 | 51.593 | 0.59 | -1.656 | -1.629 | β |
| Kharchenko et al. | 2016 | 322.607 | 51.604 | β | β | β | β |
| Dias et al. | 2014 | 322.612 | 51.6 | β | -2.3 | -0.1 | β |
| Kharchenko et al. | 2013 | 322.612 | 51.608 | β | -3.2 | 2.04 | -5.6 |
| Gozha et al. | 2012 | 322.612 | 51.6 | β | β | β | β |
| Kharchenko et al. | 2012 | 322.612 | 51.608 | β | -3.2 | 2.04 | -5.6 |
| Kharchenko et al. | 2007 | 322.6 | 51.6 | β | 0.1 | β | β |
| van den Bergh | 2006 | 322.625 | 51.583 | β | β | β | β |
| Chen et al. | 2003 | 322.627 | 51.581 | β | 0.98 | 0.22 | -5.6 |
| Dias et al. | 2002 | 322.613 | 51.6 | β | 0.98 | 0.22 | -18.95 |
| Dambis | 1999 | 322.612 | 51.6 | β | β | β | β |
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 | 1.6 | 2.36 | 2.43 | 123 | 0.085 | 2234 | 0.52 | 0.0 |
| Wei et al. | 2025 | 1.90 | 1.83 | β | 162 | 0.500 | 2234 | 0.44 | β |
| Almeida et al. | 2025 | 1.59 | 2.10 | β | 95 | β | 3064 | β | β |
| Zhang et al. | 2024 | β | β | β | β | -0.078(1) | β | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 4293(1) | β | β |
| Cavallo et al. | 2024 | 1.85 | 2.30 | β | 155 | 0.490 | β | β | β |
| Hunt & Reffert | 2023 | 1.58 | 2.22 | 2.43 | 98 | β | β | β | β |
| Almeida et al. | 2023 | 1.55 | 2.33 | β | 55 | -0.005 | 2152(1) | 0.60 | β |
| Just et al. | 2023 | β | β | β | 116 | β | 71 | β | β |
| Jaehnig et al. | 2021 | 1.60(1) | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 1.62 | 2.48 | β | 138 | β | β | β | 0 |
| Dias et al. | 2021 | 1.59 | 2.10 | β | 95 | 0.174 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 1.67 | 1.81 | β | 195 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 1.62 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 234 | -1.250 | β | β | β |
| Soubiran et al. | 2018 | 1.62 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 1.62 | β | β | β | β | β | β | β |
| Kharchenko et al. | 2016 | 1.60 | 2.39 | β | 116 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.60 | 2.39 | β | 116 | β | β | β | β |
| Gozha et al. | 2012 | 1.30 | β | β | 139 | β | β | β | β |
| Kharchenko et al. | 2012 | 1.60 | 2.39 | β | 116 | β | β | β | β |
| van den Bergh | 2006 | 1.30 | 2.51 | β | 138 | β | β | β | β |
| Chen et al. | 2003 | 1.30 | β | β | 130 | β | β | β | β |
| Dias et al. | 2002 | 1.30 | 2.50 | β | 139 | β | β | β | β |
| Dambis | 1999 | 0.94 | 2.73 | β | 79 | 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: good fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.