Collinder 37
(NGC 1220; MWSC 261; OCL 380)
0.87
UTI
0.62
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
32.3 [N/pc2]
- CN 0.62 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Collinder 37 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below 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, 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 | 99999â | 47.921 | 53.345 | 0.327 | 0.193 | -0.805 | -39.756 |
| Almeida et al. | 2025 | 47.92 | 53.346 | â | â | â | â |
| Hunt & Reffert | 2024 | 47.923 | 53.35 | 0.351 | 0.187 | -0.814 | -58.92 |
| Cavallo et al. | 2024 | 47.922 | 53.346 | 0.341 | â | â | â |
| Hunt & Reffert | 2023 | 47.923 | 53.35 | 0.351 | 0.187 | -0.814 | -58.92 |
| Almeida et al. | 2023 | 47.92 | 53.346 | â | â | â | â |
| Just et al. | 2023 | 47.91 | 53.345 | â | â | â | â |
| Jaehnig et al. | 2021 | 47.919 | 53.347 | 0.342 | 0.202 | -0.753 | â |
| Rain et al. | 2021 | 47.92 | 53.344 | 0.297 | 0.187 | -0.717 | â |
| Dias et al. | 2021 | 47.92 | 53.346 | 0.305 | 0.181 | -0.72 | â |
| Cantat-Gaudin et al. | 2020 | 47.92 | 53.344 | 0.297 | 0.187 | -0.717 | â |
| Cantat-Gaudin & Anders | 2020 | 47.92 | 53.344 | 0.297 | 0.187 | -0.717 | â |
| Bossini et al. | 2019 | 47.92 | 53.344 | â | â | â | â |
| Soubiran et al. | 2018 | 47.92 | 53.344 | â | â | â | -15.53 |
| Bica et al. | 2019 | 47.91 | 53.351 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 47.92 | 53.344 | 0.297 | 0.187 | -0.717 | â |
| Loktin & Popova | 2017 | 47.91 | 53.345 | â | -0.173 | 3.251 | â |
| Kharchenko et al. | 2016 | 47.91 | 53.345 | â | â | â | â |
| Dias et al. | 2014 | 47.917 | 53.345 | â | -0.13 | -0.5 | â |
| Kharchenko et al. | 2013 | 47.922 | 53.347 | â | 0.3 | 0.4 | â |
| Kharchenko et al. | 2012 | 47.922 | 53.347 | â | 0.3 | 0.4 | â |
| van den Bergh | 2006 | 47.925 | 53.333 | â | â | â | â |
| Dias et al. | 2002 | 47.917 | 53.345 | â | -0.13 | -0.5 | 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 | 2.805 | 2.33 | 1.56 | 85 | -0.057 | 333 | 0.54 | 0.0 |
| Almeida et al. | 2025 | 2.40 | 2.45 | â | 24 | â | 411 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 900(1) | â | â |
| Cavallo et al. | 2024 | 2.95 | 2.47 | â | 85 | 0.370 | â | â | â |
| Hunt & Reffert | 2023 | 2.70 | 2.41 | 1.56 | 114 | â | â | â | â |
| Almeida et al. | 2023 | 2.49 | 2.48 | â | 36 | -0.113 | 255(1) | 0.54 | â |
| Just et al. | 2023 | â | â | â | 158 | â | 85 | â | â |
| Jaehnig et al. | 2021 | 2.91(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 3.07 | 2.14 | â | 89 | â | â | â | 0 |
| Dias et al. | 2021 | 2.40 | 2.45 | â | 24 | -0.140 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.06 | 2.33 | â | 49 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 3.07 | â | â | â | â | â | â | â |
| Bossini et al. | 2019 | 3.19 | 2.16 | â | 91 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 3.07 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 3.07 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 3.17 | 2.07 | â | 73 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.10 | 2.33 | â | 158 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.10 | 2.33 | â | 158 | â | â | â | â |
| Kharchenko et al. | 2012 | 2.10 | 2.33 | â | 158 | â | â | â | â |
| van den Bergh | 2006 | 1.80 | 2.17 | â | 60 | â | â | â | â |
| Dias et al. | 2002 | 1.80 | 2.17 | â | 60 | 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.