Collinder 370
(NGC 6583; MWSC 2860; OCL 27; ESO 590 11; FSR 0032; FoF 152)
0.97
UTI
0.84
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
61.2 [N/pc2]
- CN 0.84 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Collinder 370 is a rich, very dense object of very 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, old 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.
Note: This object contains blue stragglers according to at least one source.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 273.96 | -22.146 | 0.403 | 1.319 | 0.088 | -2.322 |
| Li et al. | 2025 | 273.962 | -22.143 | 0.413 | 1.303 | 0.11 | β |
| Hu & Soubiran | 2025 | 273.961 | -22.14 | β | β | β | β |
| Almeida et al. | 2025 | 273.959 | -22.144 | β | β | β | β |
| Hunt & Reffert | 2024 | 273.962 | -22.145 | 0.405 | 1.329 | 0.078 | -1.512 |
| Cavallo et al. | 2024 | 273.961 | -22.14 | 0.405 | β | β | β |
| Hunt & Reffert | 2023 | 273.962 | -22.145 | 0.405 | 1.329 | 0.078 | -1.512 |
| Just et al. | 2023 | 273.945 | -22.134 | β | β | β | β |
| Jaehnig et al. | 2021 | 273.961 | -22.142 | 0.446 | 1.294 | 0.098 | β |
| Rain et al. | 2021 | 273.962 | -22.143 | 0.413 | 1.303 | 0.11 | β |
| Dias et al. | 2021 | 273.959 | -22.144 | 0.414 | 1.307 | 0.113 | -1.297 |
| Cantat-Gaudin et al. | 2020 | 273.962 | -22.143 | 0.413 | 1.303 | 0.11 | β |
| SΓ‘nchez et al. | 2020 | 273.954 | -22.137 | β | 1.504 | 0.034 | β |
| Cantat-Gaudin & Anders | 2020 | 273.962 | -22.143 | 0.413 | 1.303 | 0.11 | β |
| Liu & Pang | 2019 | 273.964 | -22.146 | 0.423 | 1.296 | 0.082 | β |
| Soubiran et al. | 2018 | 273.962 | -22.143 | β | β | β | -2.27 |
| Bica et al. | 2019 | 273.949 | -22.137 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 273.962 | -22.143 | 0.413 | 1.303 | 0.11 | β |
| Kharchenko et al. | 2016 | 273.945 | -22.134 | β | β | β | β |
| Dias et al. | 2014 | 273.954 | -22.137 | β | 0.78 | -1.56 | β |
| Kharchenko et al. | 2013 | 273.954 | -22.133 | β | -4.76 | 0.51 | 3.0 |
| Gozha et al. | 2012 | 273.954 | -22.137 | β | β | β | β |
| Dias et al. | 2002 | 273.954 | -22.137 | β | -8.75 | -6.55 | 3.0 |
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 | 2.16 | 1.79 | 1.58 | 1000 | 0.356 | 848 | β | 1.0 |
| Li et al. | 2025 | 2.20 | 1.98 | β | 754 | 0.343 | β | β | β |
| Hu & Soubiran | 2025 | β | β | β | β | -0.170(5) | β | β | β |
| Almeida et al. | 2025 | 2.16 | 1.84 | β | 940 | β | 848 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 3485(1) | β | β |
| Cavallo et al. | 2024 | 1.35 | 2.74 | β | 1445 | -0.810 | β | β | β |
| Hunt & Reffert | 2023 | 2.26 | 2.14 | 1.58 | 622 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 1000 | β | 27 | β | β |
| Jaehnig et al. | 2021 | 2.24(1) | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 2.26 | 1.58 | β | 1000 | β | β | β | 1 |
| Dias et al. | 2021 | 2.16 | 1.84 | β | 940 | 0.293 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 2.05 | 1.52 | β | 1202 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 2.26 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 550 | 0.500 | β | β | β |
| Soubiran et al. | 2018 | 2.26 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 2.26 | β | β | β | β | β | β | β |
| Kharchenko et al. | 2016 | 1.75 | 1.74 | β | 1000 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.75 | 1.74 | β | 1000 | 0.370 | β | β | β |
| Gozha et al. | 2012 | 2.10 | β | β | 1000 | 0.370 | β | β | β |
| Dias et al. | 2002 | 2.04 | 1.58 | β | 1000 | 0.370 | 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: intermediate fit. Silver sample.
Cavallo et al. (2024)
Gold sample.