Collinder 450

(NGC 7261; MWSC 3617; OCL 237; FSR 0363)

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0.96 UTI
0.78
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad) 24.1 [N/pc2]
  • CN 0.78 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 450 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, young cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is very well-studied in the literature.

(*): The parallax distance estimate (~3.63 kpc) differs significantly from the median photometric distance (~2.77 kpc).

Note: This object shares a moderate percentage of members with a later reported entry. See table with shared members information.

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

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– 335.064 58.128 0.275 -3.882 -2.941 -88.994
Li et al. 2025 335.056 58.128 0.278 -3.932 -2.909 –
Almeida et al. 2025 335.065 58.118 – – – –
Hunt & Reffert 2024 335.049 58.126 0.281 -3.877 -2.95 -142.736
Celli et al. 2024 335.056 58.128 – – – –
Cavallo et al. 2024 335.067 58.13 0.281 – – –
Hunt & Reffert 2023 335.049 58.126 0.281 -3.877 -2.95 -142.736
Just et al. 2023 335.112 58.109 – – – –
Jaehnig et al. 2021 335.071 58.126 0.305 -3.877 -2.851 –
Rain et al. 2021 335.056 58.128 0.278 -3.932 -2.909 –
Dias et al. 2021 335.065 58.118 0.275 -3.934 -2.915 –
Cantat-Gaudin et al. 2020 335.056 58.128 0.278 -3.932 -2.909 –
SΓ‘nchez et al. 2020 335.029 58.128 – -3.998 -2.745 –
Cantat-Gaudin & Anders 2020 335.056 58.128 0.278 -3.932 -2.909 –
Soubiran et al. 2018 335.056 58.128 – – – -71.34
Bica et al. 2019 335.035 58.117 – – – –
Cantat-Gaudin et al. 2018 335.056 58.128 0.278 -3.932 -2.909 –
Loktin & Popova 2017 335.025 58.127 – -1.583 -2.433 –
Kharchenko et al. 2016 335.112 58.109 – – – –
Dias et al. 2014 335.029 58.128 – -2.65 -3.37 –
Kharchenko et al. 2013 335.118 58.113 – -4.46 -7.53 –
Kharchenko et al. 2012 335.118 58.113 – -4.36 -7.54 –
van den Bergh 2006 335.1 58.083 – – – –
Dias et al. 2002 335.029 58.128 – -2.65 -3.37 –
Dambis 1999 335.029 58.128 – – – –

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– 2.765 2.825 0.96 45 0.010 1060 – 0.0
Li et al. 2025 1.45 1.52 – 1767 -0.040 – – –
Almeida et al. 2025 2.39 2.73 – 43 – 701 – –
Hunt & Reffert 2024 – – – – – 1413(1) – –
Celli et al. 2024 – – – 11 – 707 – –
Cavallo et al. 2024 3.78 2.99 – 79 0.600 – – –
Hunt & Reffert 2023 3.27 3.00 0.96 47 – – – –
Just et al. 2023 – – – 32 – 1702 – –
Jaehnig et al. 2021 3.27(1) – – – – – – –
Rain et al. 2021 3.26 2.73 – 158 – – – 0
Dias et al. 2021 2.39 2.73 – 43 0.010 – – –
Cantat-Gaudin et al. 2020 3.47 2.81 – 11 – – – –
Cantat-Gaudin & Anders 2020 3.26 – – – – – – –
Soubiran et al. 2018 3.26 – – – – – – –
Cantat-Gaudin et al. 2018 3.26 – – – – – – –
Loktin & Popova 2017 1.72 2.93 – 50 – – – –
Kharchenko et al. 2016 2.69 2.84 – 32 – – – –
Kharchenko et al. 2013 2.69 2.84 – 32 – – – –
Kharchenko et al. 2012 2.70 2.79 – 251 – – – –
van den Bergh 2006 1.68 3.01 – 47 – – – –
Dias et al. 2002 2.83 2.73 – 158 – – – –
Dambis 1999 1.50 3.26 – 20 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0177 26.2 335.05 58.13 0.3 -3.88 -2.95 -216.07 0.0

πŸ’‘ Note: The % column shows the percentage of members that Collinder 450 shares with each listed object.

Visualization

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