Alessi 8
(MWSC 2298)
0.64
UTI
0.52
CN
0.3
Cdens
0.75
CC3
0.81
Clit
1.0
Cdup
Nm (P>50%)
54
Core radius and density
1.5 [pc], 1.5 [pc-2]
- CN 0.52 Moderately populated
- Cdens 0.3 Loose
- CC3 0.75 High quality
- Clit 0.81 Well-studied
- Cdup 1.0 Unique
Overview
Alessi 8 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is 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 | 232.399 | -51.219 | 1.491 | -5.942 | -5.715 | -29.546 |
| Li et al. | 2025 | 232.408 | -51.227 | 1.479 | -5.899 | -5.729 | â |
| Almeida et al. | 2025 | 232.493 | -51.196 | â | â | â | â |
| Alfonso et al. | 2024 | 232.42 | -51.18 | 1.434 | -5.866 | -5.633 | â |
| Hunt & Reffert | 2024 | 232.298 | -51.312 | 1.482 | -6.016 | -5.702 | -32.548 |
| Cavallo et al. | 2024 | 232.503 | -51.174 | 1.489 | â | â | â |
| Hunt & Reffert | 2023 | 232.298 | -51.312 | 1.482 | -6.016 | -5.702 | -32.548 |
| Almeida et al. | 2023 | 232.515 | -51.203 | â | â | â | â |
| He et al. | 2022 | 232.276 | -51.289 | 1.494 | -6.029 | -5.684 | â |
| Tarricq et al. | 2022 | 232.355 | -51.212 | 1.494 | -5.938 | -5.683 | â |
| Richer et al. | 2021 | 232.624 | -51.271 | 1.479 | -5.914 | -5.689 | â |
| Dias et al. | 2021 | 232.493 | -51.196 | 1.479 | -5.887 | -5.736 | -26.868 |
| Cantat-Gaudin et al. | 2020 | 232.408 | -51.227 | 1.479 | -5.899 | -5.729 | â |
| Cantat-Gaudin & Anders | 2020 | 232.408 | -51.227 | 1.479 | -5.899 | -5.729 | â |
| Bossini et al. | 2019 | 232.408 | -51.227 | â | â | â | â |
| Soubiran et al. | 2018 | 232.408 | -51.227 | â | â | â | -27.26 |
| Bica et al. | 2019 | 232.393 | -51.232 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 232.408 | -51.227 | 1.479 | -5.899 | -5.729 | â |
| Dib et al. | 2018 | 232.365 | -51.255 | â | â | â | â |
| Sampedro et al. | 2017 | 232.387 | -51.233 | â | -4.94 | -4.64 | â |
| Dias et al. | 2014 | 232.388 | -51.233 | â | -5.02 | -4.58 | â |
| Piskunov et al. | 2008 | 232.384 | -51.224 | â | â | â | â |
| Piskunov et al. | 2007 | 232.384 | -51.224 | â | â | â | â |
| van den Bergh | 2006 | 232.375 | -51.208 | â | â | â | â |
| Kharchenko et al. | 2005 | 232.39 | -51.23 | â | -6.05 | -7.01 | â |
| Alessi et al. | 2003 | 232.375 | -51.208 | â | -6.1 | -5.8 | â |
| Dias et al. | 2002 | 232.387 | -51.233 | â | -6.13 | -5.8 | 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 | 0.655 | 0.28 | 0.62 | 123 | 0.035 | 113 | 0.51 | â |
| Li et al. | 2025 | 0.69 | 0.30 | â | 141 | 0.163 | â | â | â |
| Almeida et al. | 2025 | 0.67 | 0.38 | â | 143 | â | 113 | â | â |
| Alfonso et al. | 2024 | 0.67 | 0.19 | â | 132 | 0.070 | â | â | â |
| Hunt & Reffert | 2024 | 0.63 | 0.27 | 0.62 | 101 | â | 71(1) | â | â |
| Cavallo et al. | 2024 | 0.64 | 0.57 | â | 102 | -0.020 | â | â | â |
| Hunt & Reffert | 2023 | 0.63 | 0.27 | 0.62 | 101 | â | â | â | â |
| Almeida et al. | 2023 | 0.65 | 0.34 | â | 209 | -0.051 | 163(1) | 0.51 | â |
| He et al. | 2022 | â | 0.45 | â | 79 | â | â | â | â |
| Tarricq et al. | 2022 | 0.66 | â | â | 123 | â | â | â | â |
| Richer et al. | 2021 | â | 0.36 | â | 100 | â | â | â | â |
| Dias et al. | 2021 | 0.67 | 0.38 | â | 143 | 0.070 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.67 | 0.19 | â | 117 | â | â | â | â |
| Kounkel et al. | 2020 | 0.62 | 0.41 | â | 120 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.66 | â | â | â | â | â | â | â |
| Bossini et al. | 2019 | 0.66 | 0.32 | â | 137 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 0.66 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.66 | â | â | â | â | â | â | â |
| Dib et al. | 2018 | 0.71 | â | â | 127 | â | â | â | â |
| Piskunov et al. | 2008 | 0.57 | 0.28 | â | 83 | â | 176(1) | â | â |
| Piskunov et al. | 2007 | 0.57 | 0.28 | â | 83 | â | 56 | â | â |
| van den Bergh | 2006 | 0.57 | 0.28 | â | 141 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.57 | 0.28 | â | 83 | â | â | â | â |
| Alessi et al. | 2003 | 0.57 | 0.28 | â | 141 | â | â | â | â |
| Dias et al. | 2002 | 0.57 | 0.28 | â | 141 | 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: intermediate fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.99 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.99 (50th percentile).
Richer et al. (2021)
The expected number of WDs is 1.6, 1 WD candidate found, and 2 WD candidates found in the wide search.
Hu et al. (2021)
Ellipticities (core, all): e_core=0.2401, e_all=0.0537.
Bica et al. (2019)
Web updates in DAML02, some were later removed (2003 to 2010). List of clusters and alike reported by B. Alessi.