Collinder 370

(NGC 6583; MWSC 2860; OCL 27; ESO 590 11; FSR 0032; FoF 152)

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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

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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.

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

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 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 –
Hu & Soubiran 2025 273.961 -22.14 – – – –
Almeida et al. 2025 273.959 -22.144 – – – –
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 – – –
Hunt & Reffert 2023 273.962 -22.145 0.405 1.329 0.078 -1.512
Just et al. 2023 273.945 -22.134 – – – –
Jaehnig et al. 2021 273.961 -22.142 0.446 1.294 0.098 –
Rain et al. 2021 273.962 -22.143 0.413 1.303 0.11 –
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 –
SΓ‘nchez et al. 2020 273.954 -22.137 – 1.504 0.034 –
Cantat-Gaudin & Anders 2020 273.962 -22.143 0.413 1.303 0.11 –
Liu & Pang 2019 273.964 -22.146 0.423 1.296 0.082 –
Soubiran et al. 2018 273.962 -22.143 – – – -2.27
Bica et al. 2019 273.949 -22.137 – – – –
Cantat-Gaudin et al. 2018 273.962 -22.143 0.413 1.303 0.11 –
Kharchenko et al. 2016 273.945 -22.134 – – – –
Dias et al. 2014 273.954 -22.137 – 0.78 -1.56 –
Kharchenko et al. 2013 273.954 -22.133 – -4.76 0.51 3.0
Gozha et al. 2012 273.954 -22.137 – – – –
Dias et al. 2002 273.954 -22.137 – -8.75 -6.55 3.0

πŸ’‘ 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 99999– 2.16 1.79 1.58 1000 0.356 848 – 1.0
Li et al. 2025 2.20 1.98 – 754 0.343 – – –
Hu & Soubiran 2025 – – – – -0.170(5) – – –
Almeida et al. 2025 2.16 1.84 – 940 – 848 – –
Hunt & Reffert 2024 – – – – – 3485(1) – –
Cavallo et al. 2024 1.35 2.74 – 1445 -0.810 – – –
Hunt & Reffert 2023 2.26 2.14 1.58 622 – – – –
Just et al. 2023 – – – 1000 – 27 – –
Jaehnig et al. 2021 2.24(1) – – – – – – –
Rain et al. 2021 2.26 1.58 – 1000 – – – 1
Dias et al. 2021 2.16 1.84 – 940 0.293 – – –
Cantat-Gaudin et al. 2020 2.05 1.52 – 1202 – – – –
Cantat-Gaudin & Anders 2020 2.26 – – – – – – –
Liu & Pang 2019 – – – 550 0.500 – – –
Soubiran et al. 2018 2.26 – – – – – – –
Cantat-Gaudin et al. 2018 2.26 – – – – – – –
Kharchenko et al. 2016 1.75 1.74 – 1000 – – – –
Kharchenko et al. 2013 1.75 1.74 – 1000 0.370 – – –
Gozha et al. 2012 2.10 – – 1000 0.370 – – –
Dias et al. 2002 2.04 1.58 – 1000 0.370 – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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