Alessi 60
(MWSC 1071; DSH J0702.4-0108; Alessi J0702.4-0108; FoF 1395)
0.81
UTI
0.77
CN
0.85
Cdens
0.75
CC3
0.84
Clit
1.0
Cdup
Nm (P>50%)
145
Core radius and density
1.7 [pc], 4.2 [pc-2]
- CN 0.77 Rich
- Cdens 0.85 Dense
- CC3 0.75 High quality
- Clit 0.84 Well-studied
- Cdup 1.0 Unique
Overview
Alessi 60 is a rich, dense object of high C3 quality. Its parallax locates it at a moderate 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 | 99999β | 105.611 | -1.124 | 0.335 | -0.847 | -0.662 | 55.014 |
| Li et al. | 2025 | 105.619 | -1.12 | 0.336 | -0.83 | -0.653 | β |
| Almeida et al. | 2025 | 105.615 | -1.12 | β | β | β | β |
| Zhang et al. | 2024 | 105.62 | -1.12 | β | β | β | β |
| Hunt & Reffert | 2024 | 105.62 | -1.12 | 0.333 | -0.838 | -0.643 | 55.01 |
| Cavallo et al. | 2024 | 105.607 | -1.147 | 0.334 | β | β | β |
| Hunt & Reffert | 2023 | 105.62 | -1.12 | 0.333 | -0.838 | -0.643 | 55.01 |
| Just et al. | 2023 | 105.619 | -1.116 | β | β | β | β |
| Dias et al. | 2021 | 105.615 | -1.12 | 0.338 | -0.83 | -0.665 | β |
| Cantat-Gaudin et al. | 2020 | 105.619 | -1.12 | 0.336 | -0.83 | -0.653 | β |
| SΓ‘nchez et al. | 2020 | 105.625 | -1.131 | β | -0.786 | -0.689 | β |
| Zhong et al. | 2020 | 105.619 | -1.12 | β | -0.83 | -0.653 | 63.091 |
| Cantat-Gaudin & Anders | 2020 | 105.619 | -1.12 | 0.336 | -0.83 | -0.653 | β |
| Liu & Pang | 2019 | 105.617 | -1.114 | 0.338 | -0.778 | -0.495 | β |
| Bossini et al. | 2019 | 105.619 | -1.12 | β | β | β | β |
| Soubiran et al. | 2018 | 105.619 | -1.12 | β | β | β | 55.49 |
| Bica et al. | 2019 | 105.621 | -1.133 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 105.619 | -1.12 | 0.336 | -0.83 | -0.653 | β |
| Dias et al. | 2018 | β | β | β | -0.85 | -1.3 | β |
| Loktin & Popova | 2017 | 105.63 | -1.13 | β | -0.72 | -0.39 | β |
| Sampedro et al. | 2017 | 105.625 | -1.131 | β | -1.13 | -0.59 | β |
| Kharchenko et al. | 2016 | 105.619 | -1.116 | β | β | β | β |
| Dias et al. | 2014 | 105.625 | -1.131 | β | -0.96 | -1.06 | β |
| Kharchenko et al. | 2013 | 105.625 | -1.117 | β | -1.6 | -0.28 | β |
| Bukowiecki et al. | 2011 | 105.629 | -1.118 | β | β | β | β |
| Kronberger et al. | 2006 | 105.619 | -1.139 | β | β | β | β |
| Dias et al. | 2002 | 105.625 | -1.131 | β | -0.96 | -1.06 | β |
π‘ 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 | 99999β | 2.74 | 0.82 | 0.79 | 427 | 0.000 | 394 | β | β |
| Li et al. | 2025 | 2.67 | 0.65 | β | 568 | -0.125 | β | β | β |
| Almeida et al. | 2025 | 2.50 | 0.97 | β | 316 | β | 374 | β | β |
| Zhang et al. | 2024 | β | β | β | β | -0.073(1) | β | β | β |
| Hunt & Reffert | 2024 | 2.60 | 0.48 | 0.79 | 484 | β | 579(1) | β | β |
| Cavallo et al. | 2024 | 2.69 | 0.82 | β | 339 | 0.060 | β | β | β |
| Hunt & Reffert | 2023 | 2.60 | 0.48 | 0.79 | 483 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 437 | β | 144 | β | β |
| Dias et al. | 2021 | 2.50 | 0.97 | β | 316 | -0.146 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 2.95 | 0.83 | β | 224 | β | β | β | β |
| Kounkel et al. | 2020 | 2.92 | 0.81 | β | 427 | β | β | β | β |
| Zhong et al. | 2020 | 2.74(1) | 0.93 | β | 8338 | 0.000 | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 2.74 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 186 | 0.250 | β | β | β |
| Bossini et al. | 2019 | 3.18 | 0.91 | β | 218 | 0.000 | β | β | β |
| Soubiran et al. | 2018 | 2.74 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 2.74 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 4.62 | 0.50 | β | 550 | β | β | β | β |
| Kharchenko et al. | 2016 | 2.61 | 0.66 | β | 437 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.61 | 0.66 | β | 437 | β | β | β | β |
| Bukowiecki et al. | 2012 | β | β | β | β | β | 413 | β | β |
| Bukowiecki et al. | 2011 | 2.92(1) | 0.95 | β | 251 | β | β | β | β |
| Dias et al. | 2002 | 2.91 | 0.98 | β | 251 | β | β | β | β |
(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: intermediate fit.
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=0.1288, e_all=0.0778.
Bica et al. (2019)
Web updates in DAML02, some were later removed (2003 to 2010). List of clusters and alike reported by B. Alessi. The Preliminary Amateur Open Cluster Catalog, Version 08/03/2003.