Alessi 190
(UBC 5)
0.80
UTI
0.77
CN
1.0
Cdens
1.0
CC3
0.62
Clit
1.0
Cdup
Stellar density (N50/rad)
18.7 [N/pc2]
- CN 0.77 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.62 Moderately studied
- Cdup 1.0 Unique
Overview
Alessi 190 is a rich, very dense object of very 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, but with a large variance across recent sources for the absorption and age parameters (see Parameters). It is moderately studied in the literature.
Note: This object shares a significant 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 | 238.654 | -47.69 | 1.762 | -6.637 | -4.167 | -18.699 |
| Li et al. | 2025 | 238.548 | -47.74 | 1.785 | -6.695 | -4.225 | â |
| Alfonso et al. | 2024 | 238.622 | -47.68 | 1.729 | -6.618 | -4.13 | â |
| Hunt & Reffert | 2024 | 238.748 | -47.619 | 1.754 | -6.632 | -4.152 | -17.938 |
| Cavallo et al. | 2024 | 238.603 | -47.702 | 1.756 | â | â | â |
| Hunt & Reffert | 2023 | 238.748 | -47.619 | 1.754 | -6.632 | -4.152 | -17.938 |
| He et al. | 2022 | 238.711 | -47.634 | 1.756 | -6.633 | -4.144 | â |
| Tarricq et al. | 2022 | 238.674 | -47.684 | 1.762 | -6.618 | -4.13 | â |
| Cantat-Gaudin et al. | 2020 | 238.548 | -47.74 | 1.785 | -6.695 | -4.225 | â |
| Cantat-Gaudin & Anders | 2020 | 238.548 | -47.74 | 1.785 | -6.695 | -4.225 | â |
| Bica et al. | 2019 | 238.428 | -47.735 | â | â | â | â |
| Castro-Ginard et al. | 2018 | 238.429 | -47.729 | 1.788 | -6.699 | -4.184 | -14.91 |
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 | 0.55 | 0.835 | 1.64 | 209 | 0.037 | 229 | â | â |
| Li et al. | 2025 | 0.58 | 0.90 | â | 450 | 0.037 | â | â | â |
| Alfonso et al. | 2024 | 0.55 | 0.26 | â | 216 | 0.010 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 229(1) | â | â |
| Cavallo et al. | 2024 | 0.56 | 1.02 | â | 257 | 0.230 | â | â | â |
| Hunt & Reffert | 2023 | 0.53 | 0.77 | 1.64 | 175 | â | â | â | â |
| He et al. | 2022 | â | 1.20 | â | 79 | â | â | â | â |
| Tarricq et al. | 2022 | 0.54 | â | â | 209 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.55 | 0.26 | â | 200 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.55 | â | â | â | 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.