Collinder 450
(NGC 7261; MWSC 3617; OCL 237; FSR 0363)
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
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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 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 | β |
| Almeida et al. | 2025 | 335.065 | 58.118 | β | β | β | β |
| Hunt & Reffert | 2024 | 335.049 | 58.126 | 0.281 | -3.877 | -2.95 | -142.736 |
| Celli et al. | 2024 | 335.056 | 58.128 | β | β | β | β |
| Cavallo et al. | 2024 | 335.067 | 58.13 | 0.281 | β | β | β |
| Hunt & Reffert | 2023 | 335.049 | 58.126 | 0.281 | -3.877 | -2.95 | -142.736 |
| Just et al. | 2023 | 335.112 | 58.109 | β | β | β | β |
| Jaehnig et al. | 2021 | 335.071 | 58.126 | 0.305 | -3.877 | -2.851 | β |
| Rain et al. | 2021 | 335.056 | 58.128 | 0.278 | -3.932 | -2.909 | β |
| Dias et al. | 2021 | 335.065 | 58.118 | 0.275 | -3.934 | -2.915 | β |
| Cantat-Gaudin et al. | 2020 | 335.056 | 58.128 | 0.278 | -3.932 | -2.909 | β |
| SΓ‘nchez et al. | 2020 | 335.029 | 58.128 | β | -3.998 | -2.745 | β |
| Cantat-Gaudin & Anders | 2020 | 335.056 | 58.128 | 0.278 | -3.932 | -2.909 | β |
| Soubiran et al. | 2018 | 335.056 | 58.128 | β | β | β | -71.34 |
| Bica et al. | 2019 | 335.035 | 58.117 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 335.056 | 58.128 | 0.278 | -3.932 | -2.909 | β |
| Loktin & Popova | 2017 | 335.025 | 58.127 | β | -1.583 | -2.433 | β |
| Kharchenko et al. | 2016 | 335.112 | 58.109 | β | β | β | β |
| Dias et al. | 2014 | 335.029 | 58.128 | β | -2.65 | -3.37 | β |
| Kharchenko et al. | 2013 | 335.118 | 58.113 | β | -4.46 | -7.53 | β |
| Kharchenko et al. | 2012 | 335.118 | 58.113 | β | -4.36 | -7.54 | β |
| van den Bergh | 2006 | 335.1 | 58.083 | β | β | β | β |
| Dias et al. | 2002 | 335.029 | 58.128 | β | -2.65 | -3.37 | β |
| Dambis | 1999 | 335.029 | 58.128 | 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 | 2.765 | 2.825 | 0.96 | 45 | 0.010 | 1060 | β | 0.0 |
| Li et al. | 2025 | 1.45 | 1.52 | β | 1767 | -0.040 | β | β | β |
| Almeida et al. | 2025 | 2.39 | 2.73 | β | 43 | β | 701 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 1413(1) | β | β |
| Celli et al. | 2024 | β | β | β | 11 | β | 707 | β | β |
| Cavallo et al. | 2024 | 3.78 | 2.99 | β | 79 | 0.600 | β | β | β |
| Hunt & Reffert | 2023 | 3.27 | 3.00 | 0.96 | 47 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 32 | β | 1702 | β | β |
| Jaehnig et al. | 2021 | 3.27(1) | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 3.26 | 2.73 | β | 158 | β | β | β | 0 |
| Dias et al. | 2021 | 2.39 | 2.73 | β | 43 | 0.010 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 3.47 | 2.81 | β | 11 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 3.26 | β | β | β | β | β | β | β |
| Soubiran et al. | 2018 | 3.26 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 3.26 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 1.72 | 2.93 | β | 50 | β | β | β | β |
| Kharchenko et al. | 2016 | 2.69 | 2.84 | β | 32 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.69 | 2.84 | β | 32 | β | β | β | β |
| Kharchenko et al. | 2012 | 2.70 | 2.79 | β | 251 | β | β | β | β |
| van den Bergh | 2006 | 1.68 | 3.01 | β | 47 | β | β | β | β |
| Dias et al. | 2002 | 2.83 | 2.73 | β | 158 | β | β | β | β |
| Dambis | 1999 | 1.50 | 3.26 | β | 20 | 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: intermediate fit. Isochrone match: intermediate fit.
Cavallo et al. (2024)
Gold sample.