Alessi 1
(Casado Alessi 1; MWSC 88; CA 1; LeDrew 1)
0.95
UTI
0.74
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
10.9 [N/pc2]
- CN 0.74 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Alessi 1 is a moderately populated, 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 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 | 13.336 | 49.551 | 1.411 | 6.484 | -6.391 | -4.284 |
| Li et al. | 2025 | 13.343 | 49.536 | 1.39 | 6.536 | -6.245 | â |
| Hu & Soubiran | 2025 | 13.486 | 49.518 | â | â | â | â |
| Wei et al. | 2025 | 13.361 | 49.531 | 1.415 | 6.482 | -6.382 | â |
| Almeida et al. | 2025 | 13.319 | 49.536 | â | â | â | â |
| Alfonso et al. | 2024 | 13.441 | 49.442 | 1.36 | 6.369 | -6.024 | â |
| Zhang et al. | 2024 | 13.355 | 49.548 | â | â | â | â |
| Hunt & Reffert | 2024 | 13.355 | 49.548 | 1.41 | 6.47 | -6.402 | -5.191 |
| Cavallo et al. | 2024 | 13.486 | 49.518 | 1.409 | â | â | â |
| Hunt & Reffert | 2023 | 13.355 | 49.548 | 1.41 | 6.47 | -6.402 | -5.191 |
| Just et al. | 2023 | 13.318 | 49.477 | â | â | â | â |
| He et al. | 2022 | 13.356 | 49.511 | 1.411 | 6.476 | -6.42 | â |
| Tarricq et al. | 2022 | 13.283 | 49.516 | 1.424 | 6.48 | -6.435 | â |
| Dias et al. | 2021 | 13.319 | 49.536 | 1.394 | 6.548 | -6.27 | -3.343 |
| Cantat-Gaudin et al. | 2020 | 13.343 | 49.536 | 1.39 | 6.536 | -6.245 | â |
| Cantat-Gaudin & Anders | 2020 | 13.343 | 49.536 | 1.39 | 6.536 | -6.245 | â |
| Bossini et al. | 2019 | 13.343 | 49.536 | â | â | â | â |
| Soubiran et al. | 2018 | 13.343 | 49.536 | â | â | â | -3.73 |
| Bica et al. | 2019 | 13.367 | 49.57 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 13.343 | 49.536 | 1.39 | 6.536 | -6.245 | â |
| Loktin & Popova | 2017 | 13.26 | 49.765 | â | 0.857 | -4.489 | 6.0 |
| Kharchenko et al. | 2016 | 13.318 | 49.477 | â | â | â | â |
| Dias et al. | 2014 | 13.363 | 49.567 | â | 0.04 | -4.39 | â |
| Kharchenko et al. | 2013 | 13.327 | 49.48 | â | 6.13 | -7.53 | 6.0 |
| Gozha et al. | 2012 | 13.362 | 49.567 | â | â | â | â |
| Kharchenko et al. | 2012 | 13.327 | 49.48 | â | 6.13 | -7.53 | 6.0 |
| Piskunov et al. | 2008 | 13.352 | 49.571 | â | â | â | â |
| Kharchenko et al. | 2007 | 13.36 | 49.57 | â | 0.45 | â | 6.0 |
| Piskunov et al. | 2007 | 13.352 | 49.571 | â | â | â | â |
| van den Bergh | 2006 | 13.25 | 49.55 | â | â | â | â |
| Kharchenko et al. | 2005 | 13.36 | 49.57 | â | 6.51 | -7.7 | â |
| Alessi et al. | 2003 | 13.25 | 49.55 | â | 6.7 | -7.8 | â |
| Dias et al. | 2002 | 13.363 | 49.567 | â | 6.74 | -7.79 | 6.0 |
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 | 0.69 | 0.31 | 0.67 | 708 | -0.084 | 169 | 0.53 | â |
| Li et al. | 2025 | 0.67 | 0.32 | â | 1142 | -0.123 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.190(5) | â | â | â |
| Wei et al. | 2025 | 0.66 | 0.08 | â | 692 | 0.500 | 169 | 0.53 | â |
| Almeida et al. | 2025 | 0.68 | 0.42 | â | 984 | â | 87 | â | â |
| Alfonso et al. | 2024 | 0.69 | 0.08 | â | 1153 | -0.108 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.059(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 61(1) | â | â |
| Cavallo et al. | 2024 | 0.67 | 0.49 | â | 794 | 0.140 | â | â | â |
| Hunt & Reffert | 2023 | 0.66 | 0.21 | 0.67 | 748 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 692 | â | 136 | â | â |
| He et al. | 2022 | â | 0.60 | â | 501 | â | â | â | â |
| Tarricq et al. | 2022 | 0.68 | â | â | 1514 | â | â | â | â |
| Dias et al. | 2021 | 0.68 | 0.42 | â | 984 | -0.109 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.69 | 0.08 | â | 1445 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.70 | â | â | â | â | â | â | â |
| Bossini et al. | 2019 | 0.71 | 0.32 | â | 861 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 0.70 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.70 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 0.40 | 0.25 | â | 216 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.75 | 0.31 | â | 692 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.75 | 0.31 | â | 692 | â | â | â | â |
| Gozha et al. | 2012 | 0.30 | â | â | 158 | â | 324 | â | â |
| Kharchenko et al. | 2012 | 0.75 | 0.31 | â | 692 | â | â | â | â |
| Piskunov et al. | 2008 | 0.80 | 0.31 | â | 708 | â | 618(1) | â | â |
| Piskunov et al. | 2007 | 0.80 | 0.31 | â | 708 | â | 245 | â | â |
| van den Bergh | 2006 | 0.30 | 0.28 | â | 158 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.80 | 0.31 | â | 708 | â | â | â | â |
| Dias et al. | 2002 | 0.30 | 0.28 | â | 158 | 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: worst fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.