Alessi 12
(MWSC 3404; LeDrew 2; FoF 2391)
0.97
UTI
0.83
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
13.8 [N/pc2]
- CN 0.83 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Alessi 12 is a rich, very dense object of very high C3 quality. Its parallax locates it at a close 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 age, metallicity, and mass parameters (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 | 310.883 | 23.786 | 1.838 | 4.317 | -4.702 | 1.659 |
| Li et al. | 2025 | 310.875 | 23.871 | 1.816 | 4.303 | -4.639 | â |
| Wei et al. | 2025 | 310.848 | 23.812 | 1.838 | 4.315 | -4.7 | â |
| Almeida et al. | 2025 | 310.903 | 23.897 | â | â | â | â |
| Alfonso et al. | 2024 | 310.848 | 23.833 | 1.801 | 4.273 | -4.677 | â |
| Hunt & Reffert | 2024 | 310.871 | 23.538 | 1.843 | 4.277 | -4.702 | 1.244 |
| Cavallo et al. | 2024 | 310.902 | 23.873 | 1.834 | â | â | â |
| Hunt & Reffert | 2023 | 310.871 | 23.538 | 1.843 | 4.277 | -4.702 | 1.244 |
| Almeida et al. | 2023 | 310.845 | 23.933 | â | â | â | â |
| Cordoni et al. | 2023 | 310.903 | 23.897 | 1.825 | 4.329 | -4.648 | â |
| Just et al. | 2023 | 310.839 | 23.782 | â | â | â | â |
| He et al. | 2022 | 310.911 | 23.797 | 1.837 | 4.315 | -4.701 | â |
| Tarricq et al. | 2022 | 310.771 | 23.978 | 1.824 | 4.333 | -4.701 | â |
| Dias et al. | 2021 | 310.903 | 23.897 | 1.825 | 4.329 | -4.648 | -3.374 |
| Cantat-Gaudin et al. | 2020 | 310.875 | 23.871 | 1.816 | 4.303 | -4.639 | â |
| Cantat-Gaudin & Anders | 2020 | 310.875 | 23.871 | 1.816 | 4.303 | -4.639 | â |
| Liu & Pang | 2019 | 310.945 | 23.859 | 1.828 | 4.358 | -4.645 | â |
| Bossini et al. | 2019 | 310.875 | 23.871 | â | â | â | â |
| Soubiran et al. | 2018 | 310.875 | 23.871 | â | â | â | 2.43 |
| Bica et al. | 2019 | 310.873 | 23.777 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 310.875 | 23.871 | 1.816 | 4.303 | -4.639 | â |
| Loktin & Popova | 2017 | 310.95 | 23.792 | â | 4.33 | -5.35 | -26.0 |
| Kharchenko et al. | 2016 | 310.839 | 23.782 | â | â | â | â |
| Dias et al. | 2014 | 310.95 | 23.792 | â | 0.82 | -2.65 | â |
| Kharchenko et al. | 2013 | 310.845 | 23.785 | â | 3.33 | -5.28 | -26.0 |
| Gozha et al. | 2012 | 310.95 | 23.792 | â | â | â | â |
| Piskunov et al. | 2008 | 310.873 | 23.777 | â | â | â | â |
| Kharchenko et al. | 2007 | 310.95 | 23.79 | â | 0.5 | â | -26.0 |
| Piskunov et al. | 2007 | 310.873 | 23.777 | â | â | â | â |
| van den Bergh | 2006 | 310.829 | 23.775 | â | â | â | â |
| Kharchenko et al. | 2005 | 310.87 | 23.78 | â | 3.75 | -4.66 | â |
| Alessi et al. | 2003 | 310.827 | 23.775 | â | 4.3 | -5.3 | â |
| Dias et al. | 2002 | 310.95 | 23.792 | â | 4.33 | -5.35 | -26.0 |
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 | 0.54 | 0.25 | 0.92 | 123 | 0.000 | 416 | 0.23 | 0.0 |
| Li et al. | 2025 | 0.57 | 0.29 | â | 107 | -0.041 | â | â | â |
| Wei et al. | 2025 | 0.68 | 0.37 | â | 62 | 0.500 | 319 | 0.22 | â |
| Almeida et al. | 2025 | 0.54 | 0.25 | â | 157 | â | 416 | â | â |
| Alfonso et al. | 2024 | 0.53 | 0.10 | â | 133 | -0.020 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 471(1) | â | â |
| Cavallo et al. | 2024 | 0.56 | 0.47 | â | 74 | 0.040 | â | â | â |
| Hunt & Reffert | 2023 | 0.52 | 0.14 | 0.92 | 122 | â | â | â | â |
| Almeida et al. | 2023 | 0.53 | 0.27 | â | 234 | 0.003 | 485(1) | 0.48 | â |
| Cordoni et al. | 2023 | 0.54 | 0.25 | â | 157 | -0.023 | 526 | 0.23 | 0.00 |
| Just et al. | 2023 | â | â | â | 29 | â | 87 | â | â |
| He et al. | 2022 | â | 0.35 | â | 79 | â | â | â | â |
| Tarricq et al. | 2022 | 0.54 | â | â | 138 | â | â | â | â |
| Dias et al. | 2021 | 0.54 | 0.25 | â | 157 | -0.023 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.54 | 0.10 | â | 135 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.54 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 83 | 0.000 | â | â | â |
| Bossini et al. | 2019 | 0.50 | 0.21 | â | 123 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 0.54 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.54 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.11 | 0.54 | â | 238 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.54 | 0.24 | â | 29 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.54 | 0.24 | â | 29 | â | â | â | â |
| Gozha et al. | 2012 | 0.54 | â | â | 126 | â | 372 | â | â |
| Piskunov et al. | 2008 | 0.54 | 0.25 | â | 79 | â | 545(1) | â | â |
| Piskunov et al. | 2007 | 0.54 | 0.25 | â | 79 | â | 260 | â | â |
| van den Bergh | 2006 | 0.54 | 0.25 | â | 126 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.54 | 0.25 | â | 79 | â | â | â | â |
| Alessi et al. | 2003 | 0.54 | 0.25 | â | 126 | â | â | â | â |
| Dias et al. | 2002 | 0.54 | 0.25 | â | 126 | â | 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: good fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.