Alessi 22
Summary
Alessi 22 is a poorly populated, very loose object of high C3 quality. It is located at a very close distance from the Sun, below the mid-plane. It is poorly studied in the literature.
This object shares a large percentage of members with a later reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 357.029 | 36.205 | – | -3.6 | -10.5 | 7.2 |
| Hunt & Reffert (2023) | 357.172 | 36.229 | 2.804 | -4.364 | -12.792 | -5.507 |
| Cavallo et al. (2024) | 357.648 | 36.101 | 2.802 | – | – | – |
| Hu & Soubiran (2025) | 357.648 | 36.101 | – | – | – | – |
| UCC | 357.196 | 36.24 | 2.808 | -4.409 | -13.067 | -7.161 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.302, diffAV50=0.655, MOD50=7.678, logAge50=8.827 |
| Cavallo et al. (2024) | AV50=0.65, dMod50=7.69, logAge50=8.74, [Fe/H]50=-0.02 |
| Hu & Soubiran (2025) | MA22=-0.16, MA23f=-0.08, MZ23=0.07, MK24=-0.02, MF24=-0.06 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 1254 | 92.3 | 357.2 | 36.23 | 2.82 | -4.42 | -13.07 | -7.11 | 0.01 |
