Alessi 3
(MWSC 1157; FoF 2434; OCSN 137)
0.96
UTI
0.81
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
9.5 [N/pc2]
- CN 0.81 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Alessi 3 is a rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by low extinction. It is catalogued as a low-mass, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the absorption and metallicity 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 | 109.169 | -46.255 | 3.573 | -9.817 | 11.954 | 0.451 |
| Li et al. | 2025 | 109.275 | -46.142 | 3.566 | -9.875 | 11.958 | â |
| Wei et al. | 2025 | 109.212 | -46.186 | 3.611 | -9.789 | 11.957 | â |
| Almeida et al. | 2025 | 109.7 | -46.026 | â | â | â | â |
| Alfonso et al. | 2024 | 109.291 | -46.194 | 3.562 | -9.852 | 11.847 | â |
| Hunt & Reffert | 2024 | 109.187 | -46.68 | 3.575 | -9.793 | 11.916 | 0.317 |
| Cavallo et al. | 2024 | 109.175 | -46.154 | 3.575 | â | â | â |
| Hunt & Reffert | 2023 | 109.187 | -46.68 | 3.575 | -9.793 | 11.916 | 0.317 |
| Qin et al. | 2023 | 109.18 | -46.3 | 3.59 | -9.72 | 11.92 | 0.58 |
| Just et al. | 2023 | 109.046 | -46.615 | â | â | â | â |
| He et al. | 2022 | 109.09 | -46.308 | 3.611 | -9.82 | 11.958 | â |
| Tarricq et al. | 2022 | 109.341 | -46.348 | 3.619 | -9.774 | 11.954 | â |
| Dias et al. | 2021 | 109.7 | -46.026 | 3.559 | -9.872 | 12.014 | 2.314 |
| Cantat-Gaudin et al. | 2020 | 109.275 | -46.142 | 3.566 | -9.875 | 11.958 | â |
| Cantat-Gaudin & Anders | 2020 | 109.275 | -46.142 | 3.566 | -9.875 | 11.958 | â |
| Liu & Pang | 2019 | 108.974 | -46.05 | 3.558 | -9.829 | 11.977 | â |
| Soubiran et al. | 2018 | 109.275 | -46.142 | â | â | â | 0.2 |
| Bica et al. | 2019 | 109.086 | -46.61 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 109.275 | -46.142 | 3.566 | -9.875 | 11.958 | â |
| Angelo et al. | 2019 | 109.138 | -46.675 | â | â | â | â |
| Yen et al. | 2018 | 109.036 | -46.559 | 3.81 | -9.74 | 12.13 | â |
| Loktin & Popova | 2017 | 109.125 | -46.685 | â | -1.203 | 5.537 | 20.0 |
| Kharchenko et al. | 2016 | 109.046 | -46.615 | â | â | â | â |
| Dias et al. | 2014 | 109.121 | -46.685 | â | -0.4 | 5.12 | â |
| Kharchenko et al. | 2013 | 109.05 | -46.617 | â | -11.09 | 12.72 | 20.0 |
| Gozha et al. | 2012 | 109.121 | -46.685 | â | â | â | â |
| Piskunov et al. | 2008 | 109.086 | -46.61 | â | â | â | â |
| Kharchenko et al. | 2007 | 109.12 | -46.69 | â | 0.55 | â | 20.0 |
| Piskunov et al. | 2007 | 109.086 | -46.61 | â | â | â | â |
| van den Bergh | 2006 | 109.1 | -46.6 | â | â | â | â |
| Kharchenko et al. | 2005 | 109.08 | -46.61 | â | -11.63 | 12.61 | â |
| Alessi et al. | 2003 | 109.1 | -46.6 | â | -11.5 | 12.4 | â |
| Dias et al. | 2002 | 109.121 | -46.685 | â | -11.49 | 12.37 | 20.0 |
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 | 0.29 | 0.31 | 0.43 | 723 | -0.001 | 44 | 0.53 | â |
| Li et al. | 2025 | 0.29 | 0.06 | â | 946 | 0.055 | â | â | â |
| Wei et al. | 2025 | 0.26 | 0.04 | â | 832 | 0.250 | 195 | 0.53 | â |
| Almeida et al. | 2025 | 0.28 | 0.18 | â | 798 | â | 122 | â | â |
| Alfonso et al. | 2024 | 0.30 | 0.14 | â | 720 | -0.056 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 59(1) | â | â |
| Cavallo et al. | 2024 | 0.29 | 0.32 | â | 427 | 0.440 | â | â | â |
| Hunt & Reffert | 2023 | 0.27 | 0.11 | 0.43 | 625 | â | â | â | â |
| Qin et al. | 2023 | 0.27 | 0.06 | â | 891 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 741 | â | 29 | â | â |
| He et al. | 2022 | â | 0.50 | â | 398 | â | â | â | â |
| Tarricq et al. | 2022 | 0.29 | â | â | 631 | â | â | â | â |
| Dias et al. | 2021 | 0.28 | 0.18 | â | 798 | -0.057 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.30 | 0.14 | â | 631 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.28 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 437 | 0.250 | â | â | â |
| Soubiran et al. | 2018 | 0.28 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.28 | â | â | â | â | â | â | â |
| Angelo et al. | 2019 | 0.26 | â | â | 630 | â | 18 | â | â |
| Yen et al. | 2018 | 0.26 | 0.11 | â | 794 | â | â | â | â |
| Loktin & Popova | 2017 | 0.43 | 0.30 | â | 723 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.31 | 0.34 | â | 741 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.31 | 0.34 | â | 741 | -0.275 | â | â | â |
| Gozha et al. | 2012 | 0.29 | â | â | 501 | â | 37 | â | â |
| Piskunov et al. | 2008 | 0.29 | 0.34 | â | 741 | â | 52(1) | â | â |
| Piskunov et al. | 2007 | 0.29 | 0.34 | â | 741 | â | 31 | â | â |
| van den Bergh | 2006 | 0.29 | 0.34 | â | 501 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.29 | 0.34 | â | 741 | â | â | â | â |
| Alessi et al. | 2003 | 0.29 | 0.34 | â | 501 | â | â | â | â |
| Dias et al. | 2002 | 0.29 | 0.34 | â | 501 | -0.275 | 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. Gold sample.
Cavallo et al. (2024)
Gold sample.