Alessi 50
(DSH J0622.0+2104; FSR 0901)
0.65
UTI
0.8
CN
1.0
Cdens
0.62
CC3
0.4
Clit
1.0
Cdup
Stellar density (N50/rad)
20.2 [N/pc2]
- CN 0.8 Rich
- Cdens 1.0 Very dense
- CC3 0.62 Intermediate quality
- Clit 0.4 Poorly studied
- Cdup 1.0 Unique
Overview
Alessi 50 is a rich, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.
Note: This object shares a moderate percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 95.524 | 21.071 | 0.313 | 0.261 | 1.267 | 24.491 |
| Hu & Soubiran | 2025 | 95.523 | 21.077 | â | â | â | â |
| Zhang et al. | 2024 | 95.518 | 21.073 | â | â | â | â |
| Hunt & Reffert | 2024 | 95.518 | 21.073 | 0.301 | 0.267 | 1.275 | 22.436 |
| Cavallo et al. | 2024 | 95.523 | 21.077 | 0.302 | â | â | â |
| Hunt & Reffert | 2023 | 95.518 | 21.073 | 0.301 | 0.267 | 1.275 | 22.436 |
| Bica et al. | 2019 | 95.514 | 21.068 | â | â | â | â |
| Kronberger et al. | 2006 | 95.512 | 21.07 | â | â | â | 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 | 2.92 | 1.37 | 0.69 | 2312 | -0.210 | 845 | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.180(5) | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.496(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 845(1) | â | â |
| Cavallo et al. | 2024 | 2.79 | 1.56 | â | 2692 | -0.210 | â | â | â |
| Hunt & Reffert | 2023 | 3.05 | 1.18 | 0.69 | 1932 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.