Alessi 6
(MWSC 2240; FoF 2277)
0.87
UTI
0.81
CN
1.0
Cdens
0.75
CC3
0.9
Clit
1.0
Cdup
Nm (P>50%)
247
Core radius and density
1.8 [pc], 5.6 [pc-2]
- CN 0.81 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.9 Very well-studied
- Cdup 1.0 Unique
Overview
Alessi 6 is a rich, very dense object of 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 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 | 220.063 | -66.125 | 1.124 | -10.534 | -5.547 | -14.369 |
| Li et al. | 2025 | 220.058 | -66.127 | 1.1 | -10.472 | -5.559 | â |
| Almeida et al. | 2025 | 220.086 | -66.136 | â | â | â | â |
| Alfonso et al. | 2024 | 220.124 | -66.126 | 1.089 | -10.524 | -5.516 | â |
| Hunt & Reffert | 2024 | 220.011 | -66.137 | 1.126 | -10.543 | -5.535 | -14.862 |
| Cavallo et al. | 2024 | 220.066 | -66.102 | 1.13 | â | â | â |
| Hunt & Reffert | 2023 | 220.011 | -66.137 | 1.126 | -10.543 | -5.535 | -14.862 |
| Almeida et al. | 2023 | 220.006 | -66.074 | â | â | â | â |
| Just et al. | 2023 | 220.119 | -66.118 | â | â | â | â |
| He et al. | 2022 | 220.086 | -66.123 | 1.133 | -10.559 | -5.531 | â |
| Tarricq et al. | 2022 | 219.968 | -66.126 | 1.126 | -10.529 | -5.531 | â |
| Jadhav & Subramaniam | 2021 | 220.058 | -66.127 | â | â | â | â |
| Richer et al. | 2021 | 221.96 | -66.43 | 2.326 | -7.552 | -10.301 | â |
| Dias et al. | 2021 | 220.086 | -66.136 | 1.101 | -10.483 | -5.55 | -14.197 |
| Cantat-Gaudin et al. | 2020 | 220.058 | -66.127 | 1.1 | -10.472 | -5.559 | â |
| Cantat-Gaudin & Anders | 2020 | 220.058 | -66.127 | 1.1 | -10.472 | -5.559 | â |
| Liu & Pang | 2019 | 220.086 | -66.127 | 1.108 | -10.512 | -5.545 | â |
| Bossini et al. | 2019 | 220.058 | -66.127 | â | â | â | â |
| Soubiran et al. | 2018 | 220.058 | -66.127 | â | â | â | -14.35 |
| Bica et al. | 2019 | 220.07 | -66.12 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 220.058 | -66.127 | 1.1 | -10.472 | -5.559 | â |
| Dib et al. | 2018 | 220.132 | -66.12 | â | â | â | â |
| Joshi et al. | 2016 | 220.132 | -66.12 | â | â | â | â |
| Kharchenko et al. | 2016 | 220.119 | -66.118 | â | â | â | â |
| Kharchenko et al. | 2013 | 220.132 | -66.12 | â | -8.2 | -5.9 | 9.2 |
| Piskunov et al. | 2008 | 220.038 | -66.115 | â | â | â | â |
| Piskunov et al. | 2007 | 220.038 | -66.115 | â | â | â | â |
| van den Bergh | 2006 | 220.05 | -66.175 | â | â | â | â |
| Kharchenko et al. | 2005 | 220.06 | -66.12 | â | -6.2 | -6.22 | â |
| Alessi et al. | 2003 | 220.05 | -66.175 | â | -7.3 | -4.3 | 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 | 0.83 | 0.675 | 0.6 | 360 | 0.073 | 326 | 0.57 | 0 |
| Li et al. | 2025 | 0.91 | 0.68 | â | 595 | 0.244 | â | â | â |
| Almeida et al. | 2025 | 0.86 | 0.88 | â | 610 | â | 414 | â | â |
| Alfonso et al. | 2024 | 0.89 | 0.70 | â | 517 | 0.147 | â | â | â |
| Hunt & Reffert | 2024 | 0.83 | 0.67 | 0.60 | 366 | â | 496(1) | â | â |
| Cavallo et al. | 2024 | 0.89 | 0.89 | â | 417 | 0.290 | â | â | â |
| Hunt & Reffert | 2023 | 0.83 | 0.67 | 0.60 | 366 | â | â | â | â |
| Almeida et al. | 2023 | 0.86 | 1.23 | â | 421 | -0.191 | 598(1) | 0.57 | â |
| Just et al. | 2023 | â | â | â | 209 | â | 237 | â | â |
| He et al. | 2022 | â | 1.10 | â | 355 | â | â | â | â |
| Tarricq et al. | 2022 | 0.87 | â | â | 447 | â | â | â | â |
| Jadhav & Subramaniam | 2021 | 0.89 | 0.70 | â | 427 | â | 648 | â | 0(1) |
| Richer et al. | 2021 | â | 0.47 | â | 30 | â | â | â | â |
| Dias et al. | 2021 | 0.86 | 0.88 | â | 610 | 0.148 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.89 | 0.70 | â | 427 | â | â | â | â |
| Kounkel et al. | 2020 | 0.83 | 0.91 | â | 380 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.89 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 347 | 0.000 | â | â | â |
| Bossini et al. | 2019 | 0.81 | 0.72 | â | 598 | -0.382 | â | â | â |
| Soubiran et al. | 2018 | 0.89 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.89 | â | â | â | â | â | â | â |
| Dib et al. | 2018 | 0.61 | â | â | 209 | â | â | â | â |
| Joshi et al. | 2016 | 0.61 | 0.60 | â | 209 | â | 63 | â | â |
| Kharchenko et al. | 2016 | 0.61 | 0.60 | â | 209 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.61 | 0.60 | â | 209 | -0.154 | â | â | â |
| Piskunov et al. | 2008 | 0.44 | 0.60 | â | 200 | â | 64(1) | â | â |
| Piskunov et al. | 2007 | 0.44 | 0.60 | â | 200 | â | 19 | â | â |
| van den Bergh | 2006 | 0.44 | 0.60 | â | 158 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.44 | 0.60 | â | 200 | â | â | â | â |
| Alessi et al. | 2003 | 0.44 | 0.60 | â | 158 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Classified as optical pair P259, along with UPK_595.
Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.0972, e_all=0.256.
Bica et al. (2019)
Web updates in DAML02, some were later removed (2003 to 2010). List of clusters and alike reported by B. Alessi.
Dias et al. (2002)
Asterism (Alessi, B. S. 2005, private communication); cat V3.5 (Jan 2016)