Collinder 451
(NGC 7296; MWSC 3625; OCL 228; FoF 679)
0.91
UTI
0.8
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
23.8 [N/pc2]
- CN 0.8 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Collinder 451 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the mass parameter (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 | 336.986 | 52.321 | 0.378 | -2.941 | -2.748 | -30.339 |
| Li et al. | 2025 | 337.0 | 52.321 | 0.395 | -2.958 | -2.712 | â |
| Almeida et al. | 2025 | 337.003 | 52.318 | â | â | â | â |
| Hunt & Reffert | 2024 | 336.981 | 52.32 | 0.382 | -2.929 | -2.753 | -31.722 |
| Cavallo et al. | 2024 | 336.993 | 52.317 | 0.382 | â | â | â |
| Hunt & Reffert | 2023 | 336.981 | 52.32 | 0.382 | -2.929 | -2.753 | -31.722 |
| Almeida et al. | 2023 | 336.992 | 52.332 | â | â | â | â |
| Just et al. | 2023 | 337.006 | 52.326 | â | â | â | â |
| Dias et al. | 2021 | 337.003 | 52.318 | 0.399 | -2.959 | -2.712 | â |
| Cantat-Gaudin et al. | 2020 | 337.0 | 52.321 | 0.395 | -2.958 | -2.712 | â |
| Cantat-Gaudin & Anders | 2020 | 337.0 | 52.321 | 0.395 | -2.958 | -2.712 | â |
| Liu & Pang | 2019 | 336.978 | 52.32 | 0.397 | -3.002 | -2.741 | â |
| Bossini et al. | 2019 | 337.0 | 52.321 | â | â | â | â |
| Soubiran et al. | 2018 | 337.0 | 52.321 | â | â | â | -29.85 |
| Bica et al. | 2019 | 337.01 | 52.311 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 337.0 | 52.321 | 0.395 | -2.958 | -2.712 | â |
| Loktin & Popova | 2017 | 337.005 | 52.326 | â | -1.148 | -0.75 | â |
| Kharchenko et al. | 2016 | 337.006 | 52.326 | â | â | â | â |
| Dias et al. | 2014 | 337.004 | 52.323 | â | -3.16 | -2.11 | â |
| Kharchenko et al. | 2013 | 337.012 | 52.33 | â | -3.41 | -4.5 | â |
| Kharchenko et al. | 2012 | 337.012 | 52.33 | â | -3.41 | -4.5 | â |
| Dias et al. | 2002 | 337.004 | 52.323 | â | -3.16 | -2.11 | 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 | 2.365 | 0.71 | 0.53 | 324 | -0.089 | 438 | 0.54 | â |
| Li et al. | 2025 | 2.30 | 0.63 | â | 487 | -0.161 | â | â | â |
| Almeida et al. | 2025 | 2.41 | 0.78 | â | 259 | â | 234 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 833(1) | â | â |
| Cavallo et al. | 2024 | 2.32 | 0.86 | â | 324 | -0.240 | â | â | â |
| Hunt & Reffert | 2023 | 2.39 | 0.22 | 0.53 | 531 | â | â | â | â |
| Almeida et al. | 2023 | 2.41 | 0.79 | â | 251 | -0.089 | 642(1) | 0.54 | â |
| Just et al. | 2023 | â | â | â | 473 | â | 82 | â | â |
| Dias et al. | 2021 | 2.41 | 0.78 | â | 259 | -0.002 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.37 | 0.79 | â | 105 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.36 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 589 | -0.250 | â | â | â |
| Bossini et al. | 2019 | 2.60 | 0.71 | â | 84 | -0.020 | â | â | â |
| Soubiran et al. | 2018 | 2.36 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.36 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 3.15 | 0.51 | â | 4 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.01 | 0.59 | â | 473 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.01 | 0.59 | â | 473 | â | â | â | â |
| Kharchenko et al. | 2012 | 2.01 | 0.59 | â | 473 | â | â | â | â |
| Dias et al. | 2002 | 2.45 | 0.74 | â | 282 | 0.000 | 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: intermediate fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.